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1211.4742	i	we consider the statistical problem of functional linear regression ( flr ) . in its standard version , one observes the data @xmath0 where @xmath1 are i.i.d . random variables taking their values in @xmath2)$ ] , that is , the set consisting of all continuous functions on the interval @xmath3 $ ] , and @xmath4 with @x...	we consider the statistical experiment of functional linear regression ( flr ) . moreover , we show equivalence of flr and an empirical version of the white noise model for finite sample sizes . as an application , we derive sharp minimax constants in the flr model which are still valid in the case of unknown design di...	we consider the statistical experiment of functional linear regression ( flr ) . furthermore , we introduce a white noise model where one observes an it process , which contains the covariance operator of the corresponding flr model in its construction . we prove asymptotic equivalence of flr and this white noise model...
1003.1197	c	in this paper , we considered the sn shock effects , the msw effects , the collective effects , and the earth matter effects in the detection of type ii sn neutrinos . also , we considered the uncertainties in the neutrino luminosities @xmath3 , their temperatures @xmath4 , and their pinching parameters @xmath5 in the ...	we consider the supernova shock effects , the mikheyev - smirnov - wolfenstein ( msw ) effects , the collective effects , and the earth matter effects in the detection of type ii supernova neutrinos on the earth . it is found that the event number of supernova neutrinos depends on the neutrino mass hierarchy , the neut...	we consider the supernova shock effects , the mikheyev - smirnov - wolfenstein ( msw ) effects , the collective effects , and the earth matter effects in the detection of type ii supernova neutrinos on the earth . it is found that the event number of supernova neutrinos depends on the neutrino mass hierarchy , the neut...
1409.6855	i	origami manifolds appeared in differential geometry recently as a generalization of symplectic manifolds @xcite . toric origami manifolds are in turn generalizations of symplectic toric manifolds . toric origami manifolds are a special class of @xmath0-dimensional compact manifolds with an effective action of a half - ...	we construct quasitoric manifolds of dimension 6 and higher which are not equivariantly homeomorphic to any toric origami manifold . all necessary topological definitions and combinatorial constructions are given and the statement is reformulated in discrete geometrical terms . the problem reduces to existence of plana...	we construct quasitoric manifolds of dimension 6 and higher which are not equivariantly homeomorphic to any toric origami manifold . all necessary topological definitions and combinatorial constructions are given and the statement is reformulated in discrete geometrical terms . the problem reduces to existence of plana...
1105.1666	i	the equation of state ( eos ) of dense matter plays an important role in various astrophysical phenomena such as supernova explosions and the formation of neutron stars and black holes @xcite . simulations of core - collapse supernovae cover a wide range of thermodynamic conditions , and extremely high density and tem...	the study is based on the relativistic mean - field ( rmf ) theory , which can provide an excellent description of nuclear matter and finite nuclei . the thomas fermi approximation in combination with assumed nucleon distribution functions and a free energy minimization is adopted to describe the non - uniform matter ...	we construct the equation of state ( eos ) of dense matter covering a wide range of temperature , proton fraction , and density for the use of core - collapse supernova simulations . the study is based on the relativistic mean - field ( rmf ) theory , which can provide an excellent description of nuclear matter and fin...
1105.1666	r	in this work , we construct the eos tables covering a wide range of temperature @xmath34 , proton fraction @xmath19 , and baryon mass density @xmath35 for the use of core - collapse supernova simulations . we present two sets of eos tables , namely eos2 and eos3 . eos2 takes into account only the nucleon degree of free...	we construct the equation of state ( eos ) of dense matter covering a wide range of temperature , proton fraction , and density for the use of core - collapse supernova simulations . we treat the uniform matter and non - uniform matter consistently using the same rmf theory . we present two sets of eos tables , namely ...	we construct the equation of state ( eos ) of dense matter covering a wide range of temperature , proton fraction , and density for the use of core - collapse supernova simulations . the study is based on the relativistic mean - field ( rmf ) theory , which can provide an excellent description of nuclear matter and fin...
1105.1666	i	in this paper , we have presented two sets of the eos tables ( eos2 and eos3 ) covering a wide range of temperature @xmath34 , proton fraction @xmath19 , and baryon mass density @xmath35 for the use of core - collapse supernova simulations . the difference between eos2 and eos3 is that only the nucleon degree of freedo...	eos2 is an update of our earlier work published in 1998 ( eos1 ) , where only the nucleon degree of freedom is taken into account . the effect of hyperons on the eos is negligible in the low - temperature and low - density region , whereas it tends to soften the eos at high density . in comparison with eos1 , eos2 and ...	we construct the equation of state ( eos ) of dense matter covering a wide range of temperature , proton fraction , and density for the use of core - collapse supernova simulations . the study is based on the relativistic mean - field ( rmf ) theory , which can provide an excellent description of nuclear matter and fin...
hep-ph0305152	i	0.6truecm the publication of the first results of the kamland experiment marks the beginning of a new era in the studies of neutrino mixing and oscillations - the era of high precision determination of the neutrino mixing parameters . the data obtained by the solar neutrino experiments homestake , kamiokande , sage , g...	this ratio is particularly sensitive to the earth matter effects in the atmospheric neutrino oscillations , and thus to the values of and , and being the neutrino mixing angle limited by the chooz and palo verde experiments and that responsible for the dominant atmospheric ( ) oscillations . it is also sensitive to the...	we derive predictions for the nadir angle ( ) dependence of the ratio of the rates of thelike andlike multi - gev events measured in water - erenkov detectors in the case of 3-neutrino oscillations of the atmospheric ( ) and ( ) , driven by one neutrino mass squared difference , . this ratio is particularly sensitive t...
hep-ph0305152	r	0.6truecm the results of our analysis are summarized graphically in figs . 1 - 5 . we have used in the calculations the predictions for the nadir angle and energy distributions of the atmospheric neutrino fluxes given in @xcite . in this analysis , we only consider deep inelastic scattering ( dis ) cross sections and w...	we derive predictions for the nadir angle ( ) dependence of the ratio of the rates of thelike andlike multi - gev events measured in water - erenkov detectors in the case of 3-neutrino oscillations of the atmospheric ( ) and ( ) , driven by one neutrino mass squared difference , . we show that for , and at , the earth ...	we derive predictions for the nadir angle ( ) dependence of the ratio of the rates of thelike andlike multi - gev events measured in water - erenkov detectors in the case of 3-neutrino oscillations of the atmospheric ( ) and ( ) , driven by one neutrino mass squared difference , . this ratio is particularly sensitive t...
1702.06545	c	this paper presents a physical mechanism that may enable detection of inclined water maser disks orbiting massive black holes via the lensing / deflection of in - going systemic masers . the observational signature of an inclined disk is a maser line or line complex with limited doppler extent that appears to arise at ...	. the signature of an inclined water maser disk would be narrow masers near the systemic velocity that appear to emit from the black hole position , as identified by the radio continuum core . to explore this possibility , we present high resolution ( 0.070.17 ) very large array line and continuum observations of 13 ga...	we describe a method to identify inclined water maser disks orbiting massive black holes and to potentially use them to measure black hole masses . due to the geometry of maser amplification pathways , the minority of water maser disks are observable : only those viewed nearly edge - on have been identified , suggestin...
1612.09382	i	convex algebraic geometry studies convex hulls of semialgebraic sets @xcite . the convex hull of finitely many points , a zero - dimensional variety , is a polytope @xcite . polytopes have finitely many faces , which are themselves polytopes . the boundary of the convex hull of a higher - dimensional algebraic set ty...	we describe convex hulls of the simplest compact space curves , reducible quartics consisting of two circles . when the circles do not meet in complex projective space , their algebraic boundary contains an irrational ruled surface of degree eight whose ruling forms a genus one curve . we classify which curves arise , ...	we describe convex hulls of the simplest compact space curves , reducible quartics consisting of two circles . when the circles do not meet in complex projective space , their algebraic boundary contains an irrational ruled surface of degree eight whose ruling forms a genus one curve . we classify which curves arise , ...
1405.4883	i	the surface code @xcite is one of the simplest and most studied quantum error correcting codes . it can be realized on a two - dimensional grid of qubits such that the codespace is defined by simple four - qubit parity check operators acting on nearest - neighbor qubits . recent years have witnessed a surge of interes...	we describe two implementations of the optimal error correction algorithm known as the maximum likelihood decoder ( mld ) for the 2d surface code with a noiseless syndrome extraction . first , we show how to implement mld exactly in time , where is the number of code qubits . this reduction however requires a special n...	we describe two implementations of the optimal error correction algorithm known as the maximum likelihood decoder ( mld ) for the 2d surface code with a noiseless syndrome extraction . first , we show how to implement mld exactly in time , where is the number of code qubits . our implementation uses a reduction from ml...
1307.2896	i	the processes in the interstellar medium ( ism , or gas ) that determine its distribution , structure , and the formation of stars are multiple , very complex , and operate on atomic to galactic size scales ( see e.g. * ? ? ? this makes it difficult to develop a comprehensive model for the distribution of gas and star ...	our tests focus on intermediate radii ( 0.3 to 1 times the optical radius ) because there are insufficient data to test the outer disks and the fits are less accurate in detail in the centre . to optimise the model , we evaluate four recipes for the stability parameter , three recipes for apportioning the ism into mole...	we develop a model for the distribution of the ism and star formation in galaxies based on recent studies that indicate that galactic disks stabilise to a constant stability parameter , which we combine with prescriptions of how the phases of the ism are determined and for the star formation law ( sfl ) . the model pre...
1307.2896	i	we have developed a simple ` constant @xmath3 disk ' ( cq - disk ) model for predicting the distribution of ism and star formation in galaxies based on the assumption that the two - fluid instability parameter ( @xmath0 ) of the galactic disk is a constant . the model predicts the gas surface mass density and star form...	we develop a model for the distribution of the ism and star formation in galaxies based on recent studies that indicate that galactic disks stabilise to a constant stability parameter , which we combine with prescriptions of how the phases of the ism are determined and for the star formation law ( sfl ) . the model pre...	we develop a model for the distribution of the ism and star formation in galaxies based on recent studies that indicate that galactic disks stabilise to a constant stability parameter , which we combine with prescriptions of how the phases of the ism are determined and for the star formation law ( sfl ) . the model pre...
1208.3481	i	quantum liquids are among the most sought after states of matter . one celebrated class of such quantum liquids , the fractional quantum - hall ( fqh ) states , @xcite has been a locus of scientific attention for almost three decades . initially introduced to explain the fractional quantum - hall effect ( fqhe ) obser...	we analyze how very flat single - particle bands with non - trivial topological character , a chern number , arise both in the limit of infinite on - site interactions as well as in more realistic regimes . exact diagonalization is then used to investigate an effective one - orbital spinless - fermion model at fraction...	we discuss the low - energy limit of three - orbital kondo - lattice and hubbard models describing orbitals on a triangular lattice near half - filling . we analyze how very flat single - particle bands with non - trivial topological character , a chern number , arise both in the limit of infinite on - site interaction...
1208.3481	r	the interacting hamiltonian can be diagonalized exactly for small systems , using the lanczos method . @xcite unless otherwise noted , the results presented here are on a @xmath138 unit - cell torus ( i.e. , @xmath139 real - space sites ) . we do not project onto the flat subband , see fig . [ fig : disp](a ) , but ins...	it is shown that fci states are robust against disorder in the underlying magnetic texture that defines the topological character of the band . we also investigate competition between a fci state and a charge density wave ( cdw ) and discuss the effects of particle - hole asymmetry and fermi - surface nesting . neverth...	we discuss the low - energy limit of three - orbital kondo - lattice and hubbard models describing orbitals on a triangular lattice near half - filling . we analyze how very flat single - particle bands with non - trivial topological character , a chern number , arise both in the limit of infinite on - site interaction...
1208.3481	i	based on an earlier investigation , @xcite we have illustrated extensively how fci states can emerge in a strongly correlated multiorbital model and have shown how an effective spinless one - orbital model with nearly flat bands and non - zero chern number @xmath1 arises as the the low - energy limit of kondo - lattic...	we discuss the low - energy limit of three - orbital kondo - lattice and hubbard models describing orbitals on a triangular lattice near half - filling . fci states turn out to be rather robust and do not require very flat bands , but can also arise when filling or an absence of fermi - surface nesting disfavor the com...	we discuss the low - energy limit of three - orbital kondo - lattice and hubbard models describing orbitals on a triangular lattice near half - filling . we analyze how very flat single - particle bands with non - trivial topological character , a chern number , arise both in the limit of infinite on - site interaction...
1212.3503	i	in a @xmath0-dimensional hilbert space @xmath3 , the description of any quantum state @xmath4 generated by a source can be obtained by quantum tomography . for any density matrix @xmath4 , which is hermitian and has trace @xmath5 , @xmath6 independent measurements are sufficient and necessary to uniquely specify @xmath...	we consider two different types of uniqueness : ( 1 ) no other pure state is compatible with the same measurement results and ( 2 ) no other state , pure or mixed , is compatible with the same measurement results . for case ( 1 ) , it was known that for a-dimensional hilbert space , there exists a set of observables th...	we discuss the uniqueness of quantum states compatible with given measurement results for a set of observables . for a given pure state , we consider two different types of uniqueness : ( 1 ) no other pure state is compatible with the same measurement results and ( 2 ) no other state , pure or mixed , is compatible wit...
1212.3503	i	in this section we discuss the case where the hilbert space @xmath3 is a multipartite quantum system , where the observables correspond to the reduced density matrices ( rdms ) . that is , the observables are chosen to be acting nontrivially only on some subsystems . for instance , for a three - qubit system , the obse...	unique determination of a pure state by its reduced density matrices ( rdms ) , a special case of determination by observables , is also discussed . we improve the best known bound on local dimensions in which almost all pure states are uniquely determined by their rdms for case ( 2 ) .	we discuss the uniqueness of quantum states compatible with given measurement results for a set of observables . for a given pure state , we consider two different types of uniqueness : ( 1 ) no other pure state is compatible with the same measurement results and ( 2 ) no other state , pure or mixed , is compatible wit...
astro-ph0609079	c	as a starting point for this discussion , we summarize the two main findings thus far , both of which concern dependencies of the measured color - magnitude slope on external factors : ( 1 ) the slope for the blue gcs decreases gradually towards fainter host galaxy luminosities , whereas there is no significant color -...	there is no correlation between and for gcs belonging to the red subpopulation . we identify two environmental dependencies which influence the derived color - magnitude relation : ( 1 ) the slope of the color - magnitude relation decreases in significance with decreasing galaxy luminosity , although it remains detecta...	we examine the correlation between globular cluster ( gc ) color and magnitude using hst / acs imaging for a sample of 79 early - type galaxies ( mag ) with accurate surface - brightness fluctuation distances from the acs virgo cluster survey . using the mixture modeling algorithm , we find a highly significant correla...
astro-ph0609079	i	in this paper we have analysed the color - magnitude relation for the gc subpopulations in early - type galaxies belonging to the virgo cluster . our sample consists of 79 galaxies , spanning the range @xmath0 mag , drawn from the acs virgo cluster survey ( ct 2004 ) . our principal findings can be summarized as follo...	we examine the correlation between globular cluster ( gc ) color and magnitude using hst / acs imaging for a sample of 79 early - type galaxies ( mag ) with accurate surface - brightness fluctuation distances from the acs virgo cluster survey . using the mixture modeling algorithm , we find a highly significant correla...	we examine the correlation between globular cluster ( gc ) color and magnitude using hst / acs imaging for a sample of 79 early - type galaxies ( mag ) with accurate surface - brightness fluctuation distances from the acs virgo cluster survey . using the mixture modeling algorithm , we find a highly significant correla...
1309.5716	i	thermodynamics and quantum optics have been intertwined since the inception of field quantization @xcite . over the years their interconnection has been repeatedly revealed , e.g. , in the derivation of the maser efficiency from thermodynamics @xcite and its extension to the micromaser @xcite , in suggestions to boost ...	we explore the dependence of the performance bounds of heat engines and refrigerators on the _ initial quantum state _ and the subsequent evolution of their piston , modeled by a quantized harmonic oscillator . our goal is to provide a fully quantized treatment of _ self - contained ( autonomous ) _ heat machines , as ...	we explore the dependence of the performance bounds of heat engines and refrigerators on the _ initial quantum state _ and the subsequent evolution of their piston , modeled by a quantized harmonic oscillator . our goal is to provide a fully quantized treatment of _ self - contained ( autonomous ) _ heat machines , as ...
1309.5716	r	the fully quantum autonomous heat engine whose work extraction is determined by nonpassivity should be able to reproduce in the semiclassical limit the power extraction of an externally ( _ parametrically _ ) modulated heat engine ( proposed in @xcite ) that obeys the cyclic work definition [ 14 ] ( eq.(1 ) ) , and is ...	by contrast , there is no external time - dependent driving . instead , the evolution is caused by the stationary simultaneous interaction of two heat baths ( having distinct spectra and temperatures ) with a single two - level system that is in turn coupled to the quantum piston .	we explore the dependence of the performance bounds of heat engines and refrigerators on the _ initial quantum state _ and the subsequent evolution of their piston , modeled by a quantized harmonic oscillator . our goal is to provide a fully quantized treatment of _ self - contained ( autonomous ) _ heat machines , as ...
1211.6506	c	the recent neutrino oscillation experimental highlights : ( i ) rather large value of reactor mixing angle @xmath22 and ( ii ) indication of significant deviation of the atmospheric neutrino mixing angle @xmath7 from maximality may change our theoretical approach for constructing neutrino mass models . in this paper , ...	the first pattern is proposed by two of us and is favored if the atmospheric mixing angle lies in the first octant , while the second one is preferred for the second octant of . in order to reproduce the second texture , we find that the flavor symmetry should be , while for the first pattern the flavor symmetry should...	we explore two bilarge neutrino mixing anztze within the context of abelian flavor symmetry theories : ( ) , , , and ( ) , , . the first pattern is proposed by two of us and is favored if the atmospheric mixing angle lies in the first octant , while the second one is preferred for the second octant of . in order to rep...
1409.6487	i	eccentric discs , in which the dominant motion consists of elliptical keplerian orbits , occur in a wide variety of astrophysical situations . for example , an eccentric gaseous disc is formed directly when a star ( or a giant planet ) evolves , through scattering or secular interaction , on to an orbit that closely ap...	we formulate a local dynamical model of an eccentric disc in which the dominant motion consists of elliptical keplerian orbits . the simplest solutions of the local model are laminar flows consisting of a ( generally nonlinear ) vertical oscillation of the disc . we also derive the linear evolutionary equations for an ...	we formulate a local dynamical model of an eccentric disc in which the dominant motion consists of elliptical keplerian orbits . the model is a generalization of the well known shearing sheet , and is suitable for both analytical and computational studies of the local dynamics of eccentric discs . it is spatially homog...
1409.6487	c	although keplerian discs are usually assumed to be circular , the general keplerian disc is elliptical , in accordance with kepler s first law . as found by @xcite and other authors , viscosity ( and other dissipative effects ) do not necessarily lead to the circularization of a disc , even though circular orbits have ...	the model is a generalization of the well known shearing sheet , and is suitable for both analytical and computational studies of the local dynamics of eccentric discs . we discuss the properties of the laminar solutions , showing that they can exhibit extreme compressional behaviour for eccentricities greater than abo...	we formulate a local dynamical model of an eccentric disc in which the dominant motion consists of elliptical keplerian orbits . the model is a generalization of the well known shearing sheet , and is suitable for both analytical and computational studies of the local dynamics of eccentric discs . it is spatially homog...
0910.3456	i	in this paper , we give a definition of _ coherent tangent bundles _ , which is an intrinsic formulation of wave fronts . the advantage of this formulation is that the first fundamental forms and the third fundamental forms satisfy exactly the same conditions for wave fronts in space forms , and they can reverse roles ...	are considered as induced metrics of certain homomorphisms between vector bundles . they satisfy the completely same conditions , and so can reverse roles with each other . for a given wave front of a-manifold , there are two gauss - bonnet formulas . by exchanging the roles of the fundamental forms , we get two new ad...	we give a definition of ` coherent tangent bundles ' , which is an intrinsic formulation of wave fronts . in our application of coherent tangent bundles for wave fronts , the first fundamental forms and the third fundamental forms are considered as induced metrics of certain homomorphisms between vector bundles . they ...
astro-ph0311152	c	the aim of this paper is not necessarily to ` drive a wedge ' between the ` canonical ' black hole sxts and this sub - class of low / hard state x - ray transients ( lhxt ; we note that the term ` hard x - ray transient ' has been applied previously to the be + neutron star binary systems ) . while we can see that the ...	comparison of the lightcurve morphologies , spectral behaviour , properties of the quasi - periodic oscillations and the radio jet provides the first study of such objects as a sub - class of x - ray transients . however rather than assuming that these hard state x - ray transients are different from the ` canonical ' ...	we have accumulated multiwavelength ( x - ray , optical , radio ) lightcurves for the eight black hole x - ray binaries which have been observed to enter a supposed ` soft x - ray transient ' outburst , but remained in the low / hard state throughout the outburst . comparison of the lightcurve morphologies , spectral b...
astro-ph0311152	c	we have accumulated multiwavelength datasets for the eight black hole x - ray binaries which have been observed to enter an outburst but remained in the low / hard state throughout . we show that , despite very similar x - ray spectral properties , the lightcurve morphologies of these sources are very different , as ar...	we have accumulated multiwavelength ( x - ray , optical , radio ) lightcurves for the eight black hole x - ray binaries which have been observed to enter a supposed ` soft x - ray transient ' outburst , but remained in the low / hard state throughout the outburst .	we have accumulated multiwavelength ( x - ray , optical , radio ) lightcurves for the eight black hole x - ray binaries which have been observed to enter a supposed ` soft x - ray transient ' outburst , but remained in the low / hard state throughout the outburst . comparison of the lightcurve morphologies , spectral b...
1212.1226	i	comets are understood to be frozen remnants from the formation of our solar system . as such , their chemical composition is of great significance to understanding the origin of the planets and the distribution of important molecules , including water , throughout the solar system . this was and is a major goal of the ...	we have adapted coupled escape probability , a new exact method of solving radiative transfer problems , for use in asymmetrical spherical situations . our model is intended specifically for use in modeling optically thick cometary comae , although not limited to such use . this method enables the accurate modeling of ...	we have adapted coupled escape probability , a new exact method of solving radiative transfer problems , for use in asymmetrical spherical situations . our model is intended specifically for use in modeling optically thick cometary comae , although not limited to such use . this method enables the accurate modeling of ...
astro-ph0607616	i	following on the discovery of the anomalous absorption of the cosmic microwave background ( cmb ) at 4.83 ghz by gas - phase ortho - formaldehyde ( h@xmath0co ) molecules in a few nearby galactic dark nebula @xcite , several surveys were carried out in hopes of establishing the general galactic distribution of distant ...	we have carried out a blind search in the general direction of the galactic anticenter for absorption of the cosmic microwave background ( cmb ) radiation near 4.83 ghz by molecular clouds containing gaseous ortho - formaldehyde ( hco ) . the observations were done using the 25-m radio telescope at onsala in sweden , a...	we have carried out a blind search in the general direction of the galactic anticenter for absorption of the cosmic microwave background ( cmb ) radiation near 4.83 ghz by molecular clouds containing gaseous ortho - formaldehyde ( hco ) . the observations were done using the 25-m radio telescope at onsala in sweden , a...
astro-ph0607616	c	* we have successfully detected anomalous cmb absorption by h@xmath0co - bearing dust clouds at @xmath4 of our blind survey positions in the direction of the outer galaxy . no emission profiles were found . * our success is likely due to the large improvement in sensitivity of our observations over that of earlier surv...	we have detected hco cmb absorption at of the survey pointings . although these two tracers are expected to have similar excitation requirements on the microscopic level characteristic of warm , tk , dense , condensations in molecular clouds , the co(1 - 0 ) line is expected to be optically thick , whereas the hco li...	we have carried out a blind search in the general direction of the galactic anticenter for absorption of the cosmic microwave background ( cmb ) radiation near 4.83 ghz by molecular clouds containing gaseous ortho - formaldehyde ( hco ) . the observations were done using the 25-m radio telescope at onsala in sweden , a...
astro-ph0601315	i	high galactic latitude molecular clouds ( hereafter hlcs ) are typically located at @xmath17b@xmath17 @xmath18 20@xmath430@xmath4 . since the gaussiun scale height of co is estimated to be @xmath3 100 pc in the inner galactic disk ( e.g. , magnani et al . 2000 ) , hlcs are likely located very close to the sun , within ...	we have carried out large scale co observations with a mm / sub - mm telescope nanten toward a far infrared loop - like structure whose angular extent is about 20 degrees around ( , ) ( 109 , ) in pegasus . its diameter corresponds to 25 pc at a distance of 100 pc , adopted from that of a star hd886 ( b2iv ) near the c...	we have carried out large scale co observations with a mm / sub - mm telescope nanten toward a far infrared loop - like structure whose angular extent is about 20 degrees around ( , ) ( 109 , ) in pegasus . its diameter corresponds to 25 pc at a distance of 100 pc , adopted from that of a star hd886 ( b2iv ) near the c...
astro-ph0601315	r	figure 1 shows the distribution of the velocity - integrated intensity map of @xmath6co emission . we defined a @xmath6co cloud as a collection of more than two contiguous observed positions whose integrated intensity exceeds 0.77 k km s@xmath20 ( 5@xmath30 ) . based on the definition , we identified 78 molecular cloud...	theco distribution is found to consist of 78 small clumpy clouds whose masses range from 0.04 to 11 , and 83% of theco clouds have very small masses less than 1.0 . co emission was detected in the region where the column density of h derived fromco is greater than 5 , corresponding tov of 1 mag , which takes into accou...	we have carried out large scale co observations with a mm / sub - mm telescope nanten toward a far infrared loop - like structure whose angular extent is about 20 degrees around ( , ) ( 109 , ) in pegasus . its diameter corresponds to 25 pc at a distance of 100 pc , adopted from that of a star hd886 ( b2iv ) near the c...
astro-ph0601315	c	we have made a large - scale survey of high galactic latitude molecular clouds in the @xmath7 = 10 lines of @xmath6co and @xmath9co toward a large scale structure located around ( @xmath1 , @xmath2 ) @xmath3 ( 109@xmath4 , @xmath545@xmath4 ) with nanten . this survey spatially resolved the distribution of molecular gas...	we find no indication of star formation in these clouds in iras point source catalog and 2mass point source catalog . the star hd886 ( b2iv ) may be the source of the mechanical luminosity via stellar winds to create shocks , forming the loop - like structure where the very low - mass clouds are embedded .	we have carried out large scale co observations with a mm / sub - mm telescope nanten toward a far infrared loop - like structure whose angular extent is about 20 degrees around ( , ) ( 109 , ) in pegasus . its diameter corresponds to 25 pc at a distance of 100 pc , adopted from that of a star hd886 ( b2iv ) near the c...
0912.1646	i	type ia supernovae ( sneia ) are currently the best cosmological tool to investigate the dark energy driving the accelerated expansion of the universe @xcite . though generally accepted as thermonuclear explosions of carbon - oxygen white dwarfs which have accreted sufficient mass from their companion , two competitive...	we have combined the large snia database of the canada - france - hawaii telescope supernova legacy survey and catalogs of galaxies with photometric redshifts , vla 1.4 ghz radio sources , and spitzer infrared sources . we also show the properties of sneia in radio and infrared galaxies suggest the hosts contain dust a...	we have combined the large snia database of the canada - france - hawaii telescope supernova legacy survey and catalogs of galaxies with photometric redshifts , vla 1.4 ghz radio sources , and spitzer infrared sources . we present eight sneia in early - type host galaxies which have counterparts in the radio and infrar...
astro-ph9909514	i	the properties of galaxy clusters play an important role in constraining cosmological parameters and models of large - scale structure formation . because clusters are the most massive collapsed aggregates in the universe , the cluster mass function and its evolution with redshift constrains the spectrum of density flu...	we have measured 492 redshifts ( 311 new ) in the direction of the poor cluster awm 7 and have identified 179 cluster members ( 73 new ) . we use two independent methods to derive a self - consistent mass profile , under the assumptions that the absorption - line galaxies are virialized and that they trace an underlyi...	we have measured 492 redshifts ( 311 new ) in the direction of the poor cluster awm 7 and have identified 179 cluster members ( 73 new ) . we use two independent methods to derive a self - consistent mass profile , under the assumptions that the absorption - line galaxies are virialized and that they trace an underlyi...
cond-mat9510150	i	the properties of strongly correlated electrons confined to a ladder ( or double chain ) and described by @xmath0-@xmath1 or hubbard models have been the subject of intensive investigation recently . the reason lies in the unusual spin liquid nature of the undoped parent system . another reason for especial interest is...	we have numerically investigated the doped- ladder using exact diagonalization . there is a simple picture of the excitation spectrum that can be continued to explain the behavior at isotropic coupling . at the ladder is phase separated into holes and a heisenberg ladder . at intermediate coupling the ground state show...	we have numerically investigated the doped- ladder using exact diagonalization . we have studied both the limit of strong inter - chain coupling and isotropic coupling . the ladder scales to the luther - emery liquid regime in the strong inter - chain coupling limit . in this strong coupling limit there is a simple pic...
0908.0638	r	irac has proved to be a very sensitive instrument , revealing previously unseen structures in the outer shells of expanded pne @xcite . since the nebulae in our sample are typically very compact and ir - bright , which is normal for their evolutionary status , their core emission dominates the inner few arcsec near the...	we have observed a small sample of hot post - agb stars with the infrared array camera ( irac ) and the infrared spectrograph ( irs ) on - board the spitzer space telescope . we obtained irs spectra to identify the chemistry of the envelopes and found that more than of the sources in our sample have mixed chemistry , s...	we have observed a small sample of hot post - agb stars with the infrared array camera ( irac ) and the infrared spectrograph ( irs ) on - board the spitzer space telescope . the stars were selected from the literature on the basis of their far - infrared excess ( i.e. , post - agb candidates ) and b spectral type ( i....
0908.0638	c	the number density of post - agb / proto - pn is estimated to be around 0.4 kpc@xmath68 . as a comparison , the density of agb stars is 15 kpc@xmath68 and of main sequence stars is @xmath102@xmath69 kpc@xmath68 @xcite . knowledge about this phase is mostly derived from a handful of objects , such as the c - rich source...	the combination of our irac observations with 2mass and iras catalog data , along with previous radio observations in the cm range ( where available ) allowed us to model the seds of our targets and find that in almost all of them at least two shells of dust at different temperatures must be present , the hot dust comp...	we have observed a small sample of hot post - agb stars with the infrared array camera ( irac ) and the infrared spectrograph ( irs ) on - board the spitzer space telescope . the stars were selected from the literature on the basis of their far - infrared excess ( i.e. , post - agb candidates ) and b spectral type ( i....
1204.1334	c	our spectroscopic studies have revealed intrinsic variability and amazing structure in the h@xmath5 line profiles caused by high velocity gas flows in the vicinity of the stars within the kh 15d system . the profiles observed during ingress and egress are distinctly different , changing from an inverse p - cygni profi...	we have obtained 48 high resolution echelle spectra of the pre - main sequence eclipsing binary system kh 15d ( v582 mon , p = 48.37 d , 0.6 , m = 0.6 m , m = 0.7 m ) . other observed variations depend on the orbital phase : the h emission line profile changes from an inverse p cygni type profile during ingress to an ...	we have obtained 48 high resolution echelle spectra of the pre - main sequence eclipsing binary system kh 15d ( v582 mon , p = 48.37 d , 0.6 , m = 0.6 m , m = 0.7 m ) . the eclipses are caused by a circumbinary disk seen nearly edge on , which at the epoch of these observations completely obscured the orbit of star b ...