text stringlengths 11 1.65k | source stringlengths 38 44 |
|---|---|
NGC 273 is a lenticular galaxy in the constellation Cetus. It was discovered on September 10, 1785 by William Herschel. | https://en.wikipedia.org/wiki?curid=51933204 |
Photopharmacology is an emerging approach in medicine in which drugs are activated and deactivated with light. The energy of light is used to change for shape and chemical properties of the drug, resulting in different biological activity. This is done to ultimately achieve control when and where drugs are active in a ... | https://en.wikipedia.org/wiki?curid=51934343 |
Oilfield scale inhibition is the process of preventing the formation of scale from blocking or hindering fluid flow through pipelines, valves, and pumps used in oil production and processing. Scale inhibitors (SIs) are a class of specialty chemicals that are used to slow or prevent scaling in water systems. Oilfield sc... | https://en.wikipedia.org/wiki?curid=51937029 |
Oilfield scale inhibition As the reservoir fluids are pumped from the ground, changes in temperature, pressure and chemical composition shift the equilibria and cause precipitation and deposition of sparingly soluble salts that build up over time with the potential of blocking vital assets in the oil production setups.... | https://en.wikipedia.org/wiki?curid=51937029 |
Oilfield scale inhibition The most common types of inorganic scales known to the oil/gas industry are carbonates and sulfates; sulfides and chlorites are often encountered. While, the solubility of most inorganic salts (NaCl, KCl, ...) increases with temperature (endothermic dissolution reaction) , some inorganic salts... | https://en.wikipedia.org/wiki?curid=51937029 |
Oilfield scale inhibition The slightest changes in pressure and temperature dissolves HCO in water according to equation (3) to form hydronium and bicarbonate (HCO) ions. The two reactions (2) and (4) describe the equilibrium between bicarbonate ions (HCO), which are highly soluble in water and calcium carbonate (CaCO)... | https://en.wikipedia.org/wiki?curid=51937029 |
Oilfield scale inhibition Due to its relatively high solubility in water, Calcium sulfate is the easiest sulfate scale to remove chemically as compared to strontium and barium sulfate. Scale crystals are initially dispersed in production systems until accumulation of stable crystals of insoluble sulfates and scale grow... | https://en.wikipedia.org/wiki?curid=51937029 |
Oilfield scale inhibition Scale inhibitors are specialty chemicals that are added to oil production systems to delay, reduce and/or prevent scale deposition. acrylic acid polymers, maleic acid polymers and phosphonates have been used extensively for scale treatment in water systems due to their excellent solubility, th... | https://en.wikipedia.org/wiki?curid=51937029 |
Oilfield scale inhibition Group (II) metal ions are commonly sequestered by SIs with the following functionalities; - Phosphonate ions (-POH) - Phosphate ions (-OPOH) - Phosphonate ions (-POH) - Sulphonate ions (-SO) - Carboxylate ions (-CO) A SI with a combination of two or more of these functional groups is more effi... | https://en.wikipedia.org/wiki?curid=51937029 |
Oilfield scale inhibition Efforts to develop more environmentally friendly SIs have been made since the late 1990s and an increasing number of such SIs are becoming commercially available. Recent environmental awareness over the past 15 years has resulted in the production and application of more environmentally friend... | https://en.wikipedia.org/wiki?curid=51937029 |
H band (infrared) In infrared astronomy, the H band refers to an atmospheric transmission window centred on 1.65 micrometres with a Full width at half maximum of 0.35 micrometres (in the near-infrared). | https://en.wikipedia.org/wiki?curid=51990624 |
J band (infrared) In infrared astronomy, the J band refers to an atmospheric transmission window (1.1 to 1.4 um) centred on 1.25 micrometres (in the near-infrared). Betelgeuse is the brightest near-IR source in the sky with a J band magnitude of −2.99. The next brightest stars in the J band are Antares (−2.7), R Doradu... | https://en.wikipedia.org/wiki?curid=51991052 |
FESOM (Finite-Element/volumE Sea ice-Ocean Model) is a multi-resolution ocean general circulation model that solves the equations of motion describing the ocean and sea ice using finite-element and finite-volume methods on unstructured computational grids. The model is developed and supported by researchers at the Alfr... | https://en.wikipedia.org/wiki?curid=51992248 |
FESOM The last release of with the finite-element dynamical core is FESOM1.4 (Wang et al., 2014). The release of AWI-CM using is by Sidorenko et al. in 2015. | https://en.wikipedia.org/wiki?curid=51992248 |
NGC 274 is a lenticular galaxy in the constellation Cetus. It is a pair of galaxies, the other being NGC 275, which it is currently interacting with. It was discovered on September 10, 1785 by William Herschel. It is roughly 120 million light-years away. | https://en.wikipedia.org/wiki?curid=51997781 |
NGC 275 is a barred spiral galaxy located approximately 63 million light-years from the Solar System in the constellation Cetus. It is one of a pair of galaxies, the other being NGC 274. It was discovered on October 9, 1828 by John Herschel. The galaxy was described as "very faint, small, round, southeastern of 2" by J... | https://en.wikipedia.org/wiki?curid=51997795 |
NGC 276 is a barred spiral galaxy located approximately 626 million light-years from the Solar System in the constellation Cetus. It was discovered in 1886 by Frank Muller and was later also observed by DeLisle Stewart. John Dreyer, creator of the New General Catalogue describes the object as "extremely faint, pretty s... | https://en.wikipedia.org/wiki?curid=51997860 |
NGC 277 is a lenticular galaxy in the constellation Cetus. It was discovered on October 8, 1864 by Heinrich d'Arrest. | https://en.wikipedia.org/wiki?curid=51998268 |
NGC 279 is a lenticular galaxy in the constellation Cetus. It was discovered on October 1, 1785 by William Herschel. | https://en.wikipedia.org/wiki?curid=51999333 |
NGC 280 is a spiral galaxy in the constellation Andromeda. It was discovered on December 5, 1785 by William Herschel. | https://en.wikipedia.org/wiki?curid=51999371 |
Infected cell protein 34.5 (ICP-34.5, ICP34.5, or GADD34) is a protein expressed by the ɣ34.5 gene in viruses such as herpes simplex virus; it blocks a cellular stress response to viral infection. It shares the C-terminal regulatory domain () with protein phosphatase 1 subunit 15A/B. When a cell is infected with a viru... | https://en.wikipedia.org/wiki?curid=52007407 |
NGC 282 is an elliptical galaxy in the constellation Pisces. It was discovered on October 13, 1879 by Édouard Stephan. | https://en.wikipedia.org/wiki?curid=52007903 |
NGC 283 is a spiral galaxy in the constellation Cetus. It was discovered on October 2, 1886 by Francis Leavenworth. | https://en.wikipedia.org/wiki?curid=52007918 |
NGC 284 is an elliptical galaxy in the constellation Cetus. It was discovered on October 2, 1886 by Francis Leavenworth. | https://en.wikipedia.org/wiki?curid=52007927 |
NGC 285 is a lenticular galaxy in the constellation Cetus. It was discovered on October 2, 1886 by Francis Leavenworth. | https://en.wikipedia.org/wiki?curid=52007945 |
NGC 286 is a lenticular galaxy in the constellation Cetus. It was discovered on October 2, 1886 by Francis Leavenworth. | https://en.wikipedia.org/wiki?curid=52007956 |
NGC 287 is a lenticular galaxy in the constellation Pisces. It was discovered on November 22, 1827 by John Herschel. | https://en.wikipedia.org/wiki?curid=52007985 |
Chen Dong (astronaut) Chen Dong (; born 12 December 1978) is a Chinese pilot and astronaut selected as part of the Shenzhou program. A fighter pilot in the People's Liberation Army Air Force, he was selected to be a CNSA astronaut in 2010. Chen was born in Luoyang, Henan on 12 December 1978 from a working-class family.... | https://en.wikipedia.org/wiki?curid=52009929 |
Chen Dong (astronaut) For his achievements on the Shenzhou 11 mission, Chen was awarded the Spaceflight Merit Medal (Third Class) along with the honorary title of "hero astronaut" on 26 December 2016 by the Central Military Commission. Chen has twin sons. | https://en.wikipedia.org/wiki?curid=52009929 |
K band (infrared) In infrared astronomy, the K band is an atmospheric transmission window centered on 2.2 μm (in the near-infrared 136 THz range). | https://en.wikipedia.org/wiki?curid=52012421 |
NGC 291 is a barred spiral galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. | https://en.wikipedia.org/wiki?curid=52019329 |
NGC 293 is a barred spiral galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. | https://en.wikipedia.org/wiki?curid=52019358 |
NGC 294 is an open cluster located in the Small Magellanic Cloud in the constellation Tucana. It was discovered on April 11, 1834 by John Herschel, although it was possibly observed on September 5, 1826 by James Dunlop. | https://en.wikipedia.org/wiki?curid=52019383 |
NGC 297 is an elliptical galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. | https://en.wikipedia.org/wiki?curid=52019423 |
NGC 298 is a spiral galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. | https://en.wikipedia.org/wiki?curid=52020068 |
NGC 299 is an open cluster of stars in the main body of the Small Magellanic Cloud – a nearby dwarf galaxy. It is located in the southern constellation of Tucana, just under 200,000 light years distant from the Sun. The cluster was discovered on August 12, 1834 by English astronomer John Herschel. The cluster is around... | https://en.wikipedia.org/wiki?curid=52020120 |
NGC 301 is a spiral galaxy located approximately 204 million light-years from the Solar System in the constellation Cetus. It was discovered in 1886 by Frank Muller. | https://en.wikipedia.org/wiki?curid=52020220 |
L band (infrared) In infrared astronomy, the L band is an atmospheric transmission window centred on 3.5 micrometres (in the mid-infrared). | https://en.wikipedia.org/wiki?curid=52022163 |
M band (infrared) In infrared astronomy, the M band is an atmospheric transmission window centred on 4.7 micrometres (in the mid-infrared). | https://en.wikipedia.org/wiki?curid=52022359 |
William Graham McIvor (1824 - 8 June 1876) was a Scottish gardener and superintendent of the Neilgherry Cinchona plantations in Ootacamund, India who was responsible for the successful introduction of cinchona plants in the Nilgiris in the 1860s. McIvor was born in Dollar in Scotland where his father John had settled a... | https://en.wikipedia.org/wiki?curid=52029639 |
William Graham McIvor The labour situation eased in 1877 due to the famine in the plains and an influx into the Niligiris. His funeral was attended by most government officers and among those present included Colonel R. H. Beddome. | https://en.wikipedia.org/wiki?curid=52029639 |
NGC 302 is a magnitude 16.6 star located in the constellation Cetus. It was recorded in 1886 by Frank Muller. | https://en.wikipedia.org/wiki?curid=52039583 |
NGC 303 is a lenticular galaxy in the constellation Cetus. It was discovered in 1886 by Francis Leavenworth. | https://en.wikipedia.org/wiki?curid=52039606 |
NGC 304 is a lenticular galaxy in the constellation Andromeda. It was discovered on October 23, 1878 by Édouard Stephan. | https://en.wikipedia.org/wiki?curid=52039643 |
William John Ansorge (6 April 1850 – 31 October 1913 at Luanda) was a physician who worked in Angola and Uganda and is known for exploring the fauna of the African region. He was posted as a medical officer in Uganda from 1895 to 1898. Several species of animals were named after him by museum taxonomists chiefly in Bri... | https://en.wikipedia.org/wiki?curid=52041518 |
William John Ansorge Ernst Hartert noted that Ansorge was a very valuable collector and contributor to the bird collection of Walter Rothschild at Tring. Hartert noted that Ansorge's knowledge of the species collected was limited and that he lacked a training in zoology. His early collections made from 1892 in Uganda w... | https://en.wikipedia.org/wiki?curid=52041518 |
NGC 307 is a lenticular galaxy in the constellation Cetus. It was discovered on September 6, 1831 by John Herschel. | https://en.wikipedia.org/wiki?curid=52048482 |
NGC 309 is a spiral galaxy in the constellation Cetus. It was discovered in 1876 by Wilhelm Tempel. | https://en.wikipedia.org/wiki?curid=52048522 |
Building block (chemistry) Building block is a term in chemistry which is used to describe a virtual molecular fragment or a real chemical compound the molecules of which possess reactive functional groups. Building blocks are used for bottom-up modular assembly of molecular architectures: nano-particles, metal-organic... | https://en.wikipedia.org/wiki?curid=52050131 |
Building block (chemistry) To be practically useful for the modular drug or drug candidate assembly, the building blocks should be either mono-functionalised or possessing selectively chemically addressable functional groups, for example, orthogonally protected. Selection criteria applied to organic functionalized mole... | https://en.wikipedia.org/wiki?curid=52050131 |
Building block (chemistry) Introduction of the fluorine into a molecule has been shown to be beneficial for its pharmacokinetic and pharmacodynamic properties, therefore, the fluorine-substituted building blocks in drug design increase the probability of finding drug leads. Other examples include natural and unnatural ... | https://en.wikipedia.org/wiki?curid=52050131 |
NGC 311 is a lenticular galaxy in the constellation Pisces. It was discovered on September 18, 1828 by John Herschel. | https://en.wikipedia.org/wiki?curid=52057576 |
NGC 312 is an elliptical galaxy / lenticular galaxy in the constellation Phoenix. It was discovered on September 5, 1836 by John Herschel. | https://en.wikipedia.org/wiki?curid=52057614 |
Jorge Muñoz Cristi (1898–1967) was a Chilean geologist active at the University of Chile. He obtained a degree in mining engineering in 1929, and stated to lecture in 1943. He was director of the Instituto de Geología in 1952. Muñoz Cristi was a student of Juan Brüggen. | https://en.wikipedia.org/wiki?curid=52058053 |
Daniel Frederik Eschricht (18 March 1798 – 22 February 1863) was a Danish zoologist, physiologist, and anatomist known as an authority on whales. He was born in Copenhagen, and studied medicine at Frederiks Hospital, graduating in 1822. He was a student of François Magendie in Paris from 1824-1825, composing a thesis o... | https://en.wikipedia.org/wiki?curid=52061383 |
NGC 314 is a lenticular galaxy in the constellation Sculptor. It was discovered on September 27, 1834 by John Herschel. | https://en.wikipedia.org/wiki?curid=52071403 |
NGC 315 is an elliptical galaxy in the constellation Pisces. It was discovered on September 11, 1784 by William Herschel. | https://en.wikipedia.org/wiki?curid=52071479 |
Eskebornite is a selenide mineral with the formula CuFeSe It crystallizes in the tetragonal system and it has a brassy colour. is sometimes found as thick tabular crystals, but is more often found intergrown with other selenides. It is part of the chalcopyrite group and forms a series with chalcopyrite. was first ident... | https://en.wikipedia.org/wiki?curid=52081652 |
Lalita Iyer is a journalist, writer and blogger based in Mumbai, India. She is the author of two books, ""I'm pregnant, not terminally ill, you idiot"" and ""The Boy Who Swallowed A Nail And Other Stories"", as well as writing two blogs: "Chickwit" and "Mommygolightly". Iyer is a graduate of the Institute of Chemical T... | https://en.wikipedia.org/wiki?curid=52090945 |
NGC 317 is a pair of interacting galaxies, consisting of a lenticular galaxy (PGC 3442) and a spiral galaxy (PGC 3345), in the constellation Andromeda. It was discovered on October 1, 1885 by Lewis Swift. | https://en.wikipedia.org/wiki?curid=52102207 |
NGC 318 is a lenticular galaxy in the constellation Pisces. It was discovered on November 29, 1850 by Bindon Stoney. | https://en.wikipedia.org/wiki?curid=52102225 |
NGC 319 is a spiral galaxy in the constellation Phoenix. It was first discovered on September 5, 1834 by John Herschel. | https://en.wikipedia.org/wiki?curid=52102251 |
NGC 320 is a spiral galaxy in the constellation Cetus. It was first discovered in 1886 by Francis Leavenworth. | https://en.wikipedia.org/wiki?curid=52102273 |
NGC 322 is a lenticular galaxy located approximately 318 million light-years from the Solar System in the constellation Phoenix. It was discovered on September 5, 1834 by John Herschel. It was described by Dreyer as "very faint, very small, round, a little brighter middle, 3 stars to west." It apparently seems to be in... | https://en.wikipedia.org/wiki?curid=52110764 |
NGC 323 is an elliptical galaxy located in the constellation Phoenix. It was discovered on October 3, 1834 by John Herschel. It was described by Dreyer as "pretty faint, small, round, brighter middle, preceding (western) of 2", the other being NGC 328. | https://en.wikipedia.org/wiki?curid=52128609 |
NGC 324 is a lenticular galaxy located in the constellation Phoenix. It was discovered on October 23, 1835 by John Herschel. It was described by Dreyer as "questionable, faint, small, stellar". | https://en.wikipedia.org/wiki?curid=52128630 |
NGC 325 is a spiral galaxy located in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "very faint, very small". | https://en.wikipedia.org/wiki?curid=52128652 |
Michael G. Rix Michael Gordon Rix is an Australian arachnologist, whose publications mainly concern spiders. , he was Principal Curator of Arachnology and Research Fellow in the Biodiversity and Geosciences Program at the Queensland Museum. He has held numerous professional appointments including President of the Socie... | https://en.wikipedia.org/wiki?curid=52131042 |
NGC 326 is a dumbbell galaxy in the constellation Pisces. It was discovered on August 24, 1865 by Heinrich d'Arrest. It was described by Dreyer as "faint, a little extended, 9th or 10th magnitude star to southeast." X-shaped (or "winged") radio galaxies are a class of extragalactic radio source that exhibit two, low-su... | https://en.wikipedia.org/wiki?curid=52135883 |
NGC 327 is a spiral galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It is described by Dreyer as "faint, small, extended." It is nearby galaxies NGC 329, NGC 325 and NGC 321. | https://en.wikipedia.org/wiki?curid=52135906 |
NGC 328 is a spiral galaxy in the constellation Phoenix. It was discovered on September 5, 1836 by John Herschel. It was described by Dreyer as "very faint, a little extended, very gradually brighter middle, following (eastern) of 2", the other being NGC 323. | https://en.wikipedia.org/wiki?curid=52135953 |
NGC 329 is a spiral galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "faint, extended." | https://en.wikipedia.org/wiki?curid=52135978 |
NGC 331 is a barred spiral galaxy in the constellation Cetus. It was discovered in 1886 by Francis Leavenworth. It was described by Dreyer as "extremely faint, very small, round, a little brighter middle, 12th magnitude star 3 arcmin northeast." There are two candidates as to which object is NGC 331: PGC 2759 or PGC 34... | https://en.wikipedia.org/wiki?curid=52136034 |
NGC 332 is a compact and/or lenticular galaxy in the constellation Pisces. It was discovered on October 22, 1886 by Lewis Swift. It was described by Dreyer as "very faint, small, round, several stars near to south." | https://en.wikipedia.org/wiki?curid=52136059 |
Leiden Bio Science Park The Leiden Bio Science park (LBSP) is the largest life sciences cluster in the Netherlands and ranks in the top five of the most successful science parks in Europe. It is part of Leiden and Oegstgeest and focuses on companies and universities in the Biotechnology sector. The park comprises 110 h... | https://en.wikipedia.org/wiki?curid=52141066 |
Boudewijn Karel Boom (1903–1980) was a Dutch botanist and author. | https://en.wikipedia.org/wiki?curid=52148685 |
Tasia Maximova Stadnichenko Taisia Maximova Stadnichenko (9 October 1894 – 26 November 1958), a Russian born geologist and chemist, whose fieldwork focused on the distribution of germanium and the minor-element content in coal. She was born in Taganash, Crimea on October 9, 1894 and died on November 26,1958 at the age ... | https://en.wikipedia.org/wiki?curid=52152136 |
NGC 333 is a lenticular galaxy located approximately 755 million light years away in the constellation Cetus. It was discovered in 1877 by Wilhelm Tempel. It has a companion galaxy, named PGC 3073571, which is presumed to be a physical pair of NGC 333. | https://en.wikipedia.org/wiki?curid=52157025 |
NGC 334 is a barred spiral galaxy in the constellation Sculptor. It was discovered on September 25, 1834 by John Herschel. It was described by Dreyer as "very faint, small, round, gradually a little brighter middle, 2 stars of 11th magnitude to south." | https://en.wikipedia.org/wiki?curid=52157121 |
NGC 1022 is a barred spiral galaxy located at approximately 66 million light years away in the constellation of Cetus. It was discovered on September 10, 1785 by William Herschel. | https://en.wikipedia.org/wiki?curid=52157981 |
Marine and Petroleum Geology is a peer-reviewed scientific journal covering marine and petroleum geology. It was established in 1984 and is published by Elsevier. The editor-in-chief is Massimo Zecchin (Istituto Nazionale di Oceanografia e di Geofisica Sperimentale) and (Max) Qinhong Hu (The University of Texas at Arli... | https://en.wikipedia.org/wiki?curid=52158722 |
Molybdenum carbide (MoC and MoC) is an extremely hard refractory ceramic material, commercially used in tool bits for cutting tools. | https://en.wikipedia.org/wiki?curid=52163569 |
Peptone water is a microbial growth medium composed of peptic digest of animal tissue and sodium chloride. The pH of the medium is 7.2±0.2 at 25 °C and is rich in tryptophan. is also a non-selective broth medium which can be used as a primary enrichment medium for the growth of bacteria. | https://en.wikipedia.org/wiki?curid=52167095 |
NGC 335 is a spiral galaxy in the constellation Cetus. It was discovered on October 9, 1885 by Francis Leavenworth. It was described by Dreyer as "very faint, pretty small, extended, brighter middle." | https://en.wikipedia.org/wiki?curid=52168274 |
NGC 336 is a spiral galaxy in the constellation Cetus. It was discovered on October 31, 1885 by Francis Leavenworth. It was described by Dreyer as "very faint, small, round, suddenly brighter middle." It is also known as PGC 3470. Despite this, sometimes it is mistakenly identified as PGC 3526. | https://en.wikipedia.org/wiki?curid=52168326 |
NGC 337 is a barred spiral galaxy in the constellation Cetus. It was discovered on September 10, 1785 by William Herschel. It was described by Dreyer as "pretty faint, large, extended, gradually a little brighter middle, 10th magnitude star 21 seconds of time to the east." | https://en.wikipedia.org/wiki?curid=52168388 |
Weed Science Society of America The (WSSA) is a nonprofit, learned society focused on weed science. It was founded in 1956. The organization promotes research, education, and extension outreach, provides science-based information to the public and policy makers, and fosters awareness of weeds and their impact on both m... | https://en.wikipedia.org/wiki?curid=52169764 |
NGC 338 is a spiral galaxy in the constellation Pisces. It was discovered in 1877 by Wilhelm Tempel. It was described by Dreyer as "very faint, very small, irregular figure, brighter middle." | https://en.wikipedia.org/wiki?curid=52178635 |
NGC 340 is a spiral galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "very faint, small, extended." | https://en.wikipedia.org/wiki?curid=52187779 |
NGC 341 is a spiral galaxy in the constellation Cetus. It was discovered on October 21, 1881 by Édouard Stephan. It was described by Dreyer as "faint, pretty large, round, a little brighter middle, mottled but not resolved." It has a companion galaxy, PGC 3627, which is sometimes called NGC 341B. For this, reason, it h... | https://en.wikipedia.org/wiki?curid=52187839 |
HE 2359-2844 is a subdwarf located approximately 800 light years away in the constellation Sculptor, with a surface temperature of approximately . Along with stars HE 1256-2738 and LS IV-14 116, forms a new group of star called heavy metal subdwarfs. contains very high levels of lead - 10,000 times more than the Sun. I... | https://en.wikipedia.org/wiki?curid=52193704 |
HE 1256-2738 is a subdwarf located approximately 1,000 light years away in the constellation Hydra, with a surface temperature of approximately . Along with stars HE 2359-2844 and LS IV-14 116, forms a new group of star called heavy metal subdwarfs. | https://en.wikipedia.org/wiki?curid=52193743 |
Cinco (crater) Cinco is a small crater in the Descartes Highlands of the Moon visited by the astronauts of Apollo 16. The crater is one of a group of five (hence the name, Spanish for "five") craters that were collectively called the Cinco craters during the Apollo 16 mission. The craters were designated "a", "b", "c",... | https://en.wikipedia.org/wiki?curid=52194820 |
NGC 342 is a lenticular galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "very faint, very small." | https://en.wikipedia.org/wiki?curid=52200124 |
NGC 343 are a pair of interacting galaxies in the constellation Cetus. It was discovered in 1886 by Frank Muller. It was described by Dreyer as "extremely faint, very small, irregularly round, suddenly brighter middle and nucleus (perhaps a star?)." | https://en.wikipedia.org/wiki?curid=52200160 |
NGC 344 is a barred spiral galaxy in the constellation Cetus. It was discovered in 1886 by Frank Muller. It was described by John Louis Emil Dreyer as "extremely faint, very small, irregularly round, suddenly brighter middle and nucleus (perhaps a star?)." | https://en.wikipedia.org/wiki?curid=52200246 |
NGC 345 is a spiral galaxy located in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "very faint, very small, gradually brighter middle." | https://en.wikipedia.org/wiki?curid=52200267 |
Dissociation rate The dissociation rate in chemistry, biochemistry, and pharmacology is the rate or speed at which a ligand dissociates from a protein, for instance, a receptor. It is an important factor in the binding affinity and intrinsic activity (efficacy) of a ligand at a receptor. The dissociation rate for a par... | https://en.wikipedia.org/wiki?curid=52203741 |
Sigma-D relation The Sigma-D relation, or Σ-D Relation, is the radio surface brightness to diameter relation of a supernova remnant. | https://en.wikipedia.org/wiki?curid=52206441 |
Ernest Olivier Joseph (January 6, 1844 – January 26, 1914) was a French entomologist and botanist, known as a specialist in fireflies (Lampyridae). He was founder and editor of the journal "Revue scientifique du Bourbonnais et du centre de la France". He was also involved in politics, serving as town councilor and late... | https://en.wikipedia.org/wiki?curid=52211130 |
Subsets and Splits
No community queries yet
The top public SQL queries from the community will appear here once available.