Gotowa bibliografia na temat „Molecular clouds”
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Artykuły w czasopismach na temat "Molecular clouds"
Sullivan, Colin H., L. M. Fissel, P. K. King, C.-Y. Chen, Z.-Y. Li i J. D. Soler. "Characterizing the magnetic fields of nearby molecular clouds using submillimeter polarization observations". Monthly Notices of the Royal Astronomical Society 503, nr 4 (16.03.2021): 5006–24. http://dx.doi.org/10.1093/mnras/stab596.
Pełny tekst źródłaClube, S. V. M. "Molecular clouds: comet factories?" International Astronomical Union Colloquium 83 (1985): 19–30. http://dx.doi.org/10.1017/s0252921100083779.
Pełny tekst źródłaBot, Caroline, Mónica Rubio, François Boulanger, Marcus Albrecht, Frank Bertoldi, Alberto D. Bolatto i Adam K. Leroy. "Tracing the cold molecular gas reservoir through dust emission in the SMC". Proceedings of the International Astronomical Union 4, S256 (lipiec 2008): 148–53. http://dx.doi.org/10.1017/s174392130802838x.
Pełny tekst źródłaBlitz, Leo. "Molecular Clouds at High z". Symposium - International Astronomical Union 144 (1991): 41–51. http://dx.doi.org/10.1017/s0074180900088896.
Pełny tekst źródłaLi, Pak Shing, i Richard I. Klein. "Magnetized interstellar molecular clouds – II. The large-scale structure and dynamics of filamentary molecular clouds". Monthly Notices of the Royal Astronomical Society 485, nr 4 (27.03.2019): 4509–28. http://dx.doi.org/10.1093/mnras/stz653.
Pełny tekst źródłaWong, Tony, Annie Hughes, Jürgen Ott, Jorge L. Pineda i Erik Muller. "The Molecular Cloud Population of the Large Magellanic Cloud". Proceedings of the International Astronomical Union 8, S292 (sierpień 2012): 71–74. http://dx.doi.org/10.1017/s1743921313000495.
Pełny tekst źródłaKörtgen, Bastian. "The turbulence driving parameter of molecular clouds in disc galaxies". Monthly Notices of the Royal Astronomical Society 497, nr 1 (24.07.2020): 1263–74. http://dx.doi.org/10.1093/mnras/staa2028.
Pełny tekst źródłaBraine, J., E. Rosolowsky, P. Gratier, E. Corbelli i K. F. Schuster. "Properties and rotation of molecular clouds in M 33". Astronomy & Astrophysics 612 (kwiecień 2018): A51. http://dx.doi.org/10.1051/0004-6361/201732405.
Pełny tekst źródłaYan, Qing-Zeng, Ji Yang, Yang Su, Yan Sun, Xin Zhou, Ye Xu, Hongchi Wang, Shaobo Zhang i Zhiwei Chen. "Dependence of Molecular Cloud Samples on Angular Resolution, Sensitivity, and Algorithms". Astronomical Journal 164, nr 2 (18.07.2022): 55. http://dx.doi.org/10.3847/1538-3881/ac77ea.
Pełny tekst źródłaKutner, Marc L., i Kathryn N. Mead. "Outer-Galaxy molecular clouds". Symposium - International Astronomical Union 106 (1985): 209–10. http://dx.doi.org/10.1017/s0074180900242460.
Pełny tekst źródłaRozprawy doktorskie na temat "Molecular clouds"
Beletsky, Yuri. "Extragalactic molecular clouds and chemistry of diffuse interstellar clouds". Diss., lmu, 2009. http://nbn-resolving.de/urn:nbn:de:bvb:19-105670.
Pełny tekst źródłaVichetti, Rafael Mário [UNESP]. "Síntese dos isótopos do monóxido de carbono no meio interestelar". Universidade Estadual Paulista (UNESP), 2009. http://hdl.handle.net/11449/91889.
Pełny tekst źródłaCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
De acordo com os resultados observacionais de condensações de nuvens moleculares escuras, grandes variações na razão 13CO/C18O são observadas quando se comparam os resultados obtidos nas condensações situadas dentro da mesma nuvem, bem como de nuvem para nuvem. O valor médio dessa razão na condensação principal de Ophiuchus é inferior a 5. Por outro lado, o valor encontrado nas condensações que estão situadas ao norte de Oph é maior que 10. Grandes diferenças também são encontradas quando se comparam os resultados observacionais de diferentes nuvens escuras, tais como Ophiuchus e Taurus, onde são observados também um decréscimo da razão C18O/C17O com o aumento da densidade. Os processos químicos e físicos que governam essas variações ainda não estão claros. Nesse sentido, o objetivo da presente proposta é analisar a influência do colapso gravitacional de condensações de nuvens moleculares escuras na síntese das moléculas CO, C17O, C18O, 13CO, 13C17O e 13C18O. Tal análise é feita com base em comparações entre modelos que consideram diferentes condições entre si, tais como, tamanho da cadeia química, velocidade de colapso, densidade inicial e processos de congelamento de espécies químicas na superfície de grãos de poeira. Os resultados obtidos mostram que o tamanho da cadeia química tem influência nas razões 13CO/C18O e C18O/C17O, mas não tanto quanto a densidade inicial e a velocidade do colapso. Além disso, o congelamento das espécies químicas nos grãos é mais significativo nos estágios mais avançados da evolução da condensação. Os modelos de condensações escuras que sofrem colapso gravitacional lento e em queda livre reproduzem satisfatoriamente as razões 13CO/C18O e C18O/C17O observadas, o que permite concluir que o colapso gravitacional pode ter um importante efeito nas referidas razões.
According to the observational results of dark molecular clouds condensations, large variations in the ratio 13CO/C18O are observed when comparing the results obtained in the condensations located within the same cloud and cloud to cloud. The average value of this ratio in the main condensation of Ophiuchus is below 5. On the other hand, the value found in the condensations that are located north of Oph is larger than 10. Large differences are also found when comparing the observational results of different dark clouds such as Ophiuchus and Taurus, in which are also found a decrease of the C18O/C17O ratio with increasing density. The chemical and physical processes that govern these variations are still unclear. In this sense, the objective of this proposal is to analyze the influence of the gravitational collapse of centrally condensed clumps of dense molecular gas in the synthesis of the CO, C17O, C18O, 13CO, 13C17O and 13C18O molecules. This analysis is based on comparisons among models that consider different condition, such as, chemical chain, initial density, speed of collapse and freezing processes of the chemical species on the surface of dust grains. The results show that the size of the chemical chain has influence on the 13CO/C18O and C18O/C17O ratios, but they are not as important as the initial density and the speed of the collapse. Furthermore, the freezing of chemical species on the grains occurs at later times of the collapse. The models of a gravitational free-fall collapsing core and of slowly contracting core with higher initial density are consistent with observations. These results indicate that the gravitational collapse of molecular cores can have an important effect in the 13CO/C18O and C18O/C17O ratios.
Brown, Ian David. "The velocity of molecular clouds". Thesis, University of Cambridge, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.293612.
Pełny tekst źródłaBretherton, Derek. "Star formation in molecular clouds". Thesis, Liverpool John Moores University, 2003. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.402927.
Pełny tekst źródłaRowles, Jonathan Henry. "The structure of molecular clouds". Thesis, University of Kent, 2011. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.544095.
Pełny tekst źródłaRichardson, Kevin John. "Submillimetre molecular line observations and modelling of molecular clouds". Thesis, Queen Mary, University of London, 1985. http://qmro.qmul.ac.uk/xmlui/handle/123456789/1705.
Pełny tekst źródłaMcElroy, Daniel. "Grain surface chemistry in molecular clouds". Thesis, Queen's University Belfast, 2013. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.602462.
Pełny tekst źródłaMorisawa, Yusuke. "Spectroscopic study of some chemically significant molecules in molecular clouds". 京都大学 (Kyoto University), 2005. http://hdl.handle.net/2433/144599.
Pełny tekst źródłaGarcía, Fuentes Pablo Fernando. "Giant Molecular Clouds in the Southern Milky Way". Tesis, Universidad de Chile, 2007. http://www.repositorio.uchile.cl/handle/2250/104575.
Pełny tekst źródłaDobbs, Clare Louise. "The formation of molecular clouds in spiral galaxies /". St Andrews, 2007. http://hdl.handle.net/10023/214.
Pełny tekst źródłaKsiążki na temat "Molecular clouds"
Serra, Guy, red. Nearby Molecular Clouds. Berlin, Heidelberg: Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/3-540-15991-6.
Pełny tekst źródłaHerrmann, Franz. Atomic oxygen in molecular clouds. Garching bei München: Max-Planck-Institut für extraterrestrische Physik, 1993.
Znajdź pełny tekst źródłaA, James R., Millar T. J. 1952- i University of Manchester. Astronomy Dept., red. Molecular clouds: The proceedings of a conference at the Department of Astronomy, University of Manchester, 26-30 March 1990. Cambridge [England]: Cambridge University Press, 1991.
Znajdź pełny tekst źródłaA, James R., Millar T. J i University of Manchester. Astronomy Dept., red. Molecular clouds: The proceedings of a conference at the Department ofAstronomy, University of Manchester, 26-30 March 1990. Cambridge (England): Cambridge Univerversity Press, 1991.
Znajdź pełny tekst źródłaUnited States. National Aeronautics and Space Administration. Scientific and Technical Information Branch., red. Molecular clouds in the Carina arm. [Washington, DC]: National Aeronautics and Space Administration, Scientific and Technical Information Branch, 1986.
Znajdź pełny tekst źródłaUnited States. National Aeronautics and Space Administration. Scientific and Technical Information Branch., red. Molecular clouds in Orion and Monoceros. [Washington, DC]: National Aeronautics and Space Administration, Scientific and Technical Information Branch, 1986.
Znajdź pełny tekst źródłaN, Mead Kathryn, University of Texas at Austin. Dept. of Astronomy, McDonald Observatory i United States. National Aeronautics and Space Administration, red. Molecular clouds in the outer galaxy. Austin, Tex: University of Texas at Austin, Dept. of Astronomy and McDonald Observatory, 1986.
Znajdź pełny tekst źródłaUnited States. National Aeronautics and Space Administration., red. Theoretical studies in interstellar cloud chemistry: Final report. [Washington, DC: National Aeronautics and Space Administration, 1993.
Znajdź pełny tekst źródłaUnited States. National Aeronautics and Space Administration., red. [Theory of grain alignment in molecular clouds]: [annual status report, 1 May 1992 - 28 Feb. 1993]. [Washington, DC: National Aeronautics and Space Administration, 1993.
Znajdź pełny tekst źródłaHanda, T. Thermal SiO and H13CO+ line observations of the dense molecular cloud G0.11-0.11 in the galactic center region. Nobeyama, Minamisaku, Nagano-ken, Japan: Nobeyama Radio Observatory of the National Astronomical Observatory, 2005.
Znajdź pełny tekst źródłaCzęści książek na temat "Molecular clouds"
Blitz, Leo, i Jonathan P. Williams. "Molecular Clouds". W The Origin of Stars and Planetary Systems, 3–28. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4509-1_1.
Pełny tekst źródłaCarraro, Giovanni. "Molecular Clouds". W UNITEXT for Physics, 319–40. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-75293-4_15.
Pełny tekst źródłaJaffe, D. T. "Warm Molecular Clouds". W Astrochemistry of Cosmic Phenomena, 311–15. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2761-5_68.
Pełny tekst źródłaReitner, Joachim. "Cosmic Molecular Clouds". W Encyclopedia of Geobiology, 292–93. Dordrecht: Springer Netherlands, 2011. http://dx.doi.org/10.1007/978-1-4020-9212-1_243.
Pełny tekst źródłaWilson, T. L., R. A. Gaume, K. J. Johnston i J. Schmid-Burgk. "Galactic Molecular Clouds". W ESO Astrophysics Symposia, 177–84. Berlin, Heidelberg: Springer Berlin Heidelberg, 1996. http://dx.doi.org/10.1007/978-3-540-69999-6_25.
Pełny tekst źródłaLebrun, F. "A synthetic view at large scale of local molecular clouds". W Nearby Molecular Clouds, 3–14. Berlin, Heidelberg: Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/3-540-15991-6_67.
Pełny tekst źródłade Vries, C. P. "Comparison of optical appearance and infrared emission of extended dust clouds". W Nearby Molecular Clouds, 20–24. Berlin, Heidelberg: Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/3-540-15991-6_69.
Pełny tekst źródłaBoulanger, F., B. Baud i G. D. van Albada. "Correlation of high galactic latitude HI and FIR emission and warm dust in the neutral interstellar medium". W Nearby Molecular Clouds, 28–32. Berlin, Heidelberg: Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/3-540-15991-6_71.
Pełny tekst źródłaUngerer, V., N. Mauron, J. Brillet i Nguyen-Quang-Rieu. "C18—O and optical observations of the Taurus cloud in front of 3C 111". W Nearby Molecular Clouds, 68–71. Berlin, Heidelberg: Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/3-540-15991-6_77.
Pełny tekst źródłaBeichman, C. A., J. P. Emerson, R. E. Jennings, S. Harris, B. Baud i E. T. Young. "IRAS observations of star formation in nearby molecular clouds". W Nearby Molecular Clouds, 95–103. Berlin, Heidelberg: Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/3-540-15991-6_83.
Pełny tekst źródłaStreszczenia konferencji na temat "Molecular clouds"
Puy, Denis, i Monique Signore. "Primordial molecular clouds". W 3 K COSMOLOGY. ASCE, 1999. http://dx.doi.org/10.1063/1.59317.
Pełny tekst źródłaPhillips, Thomas G. "Millimeter and submillimeter wave astronomy". W OSA Annual Meeting. Washington, D.C.: Optica Publishing Group, 1986. http://dx.doi.org/10.1364/oam.1986.mh3.
Pełny tekst źródłaRice, Johnathan, i Steven Federman. "THE TRANSITION FROM DIFFUSE ATOMIC CLOUDS TO DENSE MOLECULAR CLOUDS". W 73rd International Symposium on Molecular Spectroscopy. Urbana, Illinois: University of Illinois at Urbana-Champaign, 2018. http://dx.doi.org/10.15278/isms.2018.rl08.
Pełny tekst źródłaTurner, B. E. "The nature of molecular clouds". W ASTROPHYSICAL IMPLICATIONS OF THE LABORATORY STUDY OF PRESOLAR MATERIALS. ASCE, 1997. http://dx.doi.org/10.1063/1.53334.
Pełny tekst źródłaGredel, Roland. "Molecular abundances in translucent clouds". W The 50th international meeting of physical chemistry: Molecules and grains in space. AIP, 1994. http://dx.doi.org/10.1063/1.46571.
Pełny tekst źródłaYuan, Chi, i Junhan You. "MOLECULAR CLOUDS AND STAR FORMATION". W Proceedings of the 7th Guo Shoujing Summer School on Astrophysics. WORLD SCIENTIFIC, 1995. http://dx.doi.org/10.1142/9789814533935.
Pełny tekst źródłaChevalier, Roger A. "Supernova remnants in molecular clouds". W The eleventh astrophysics conference on young supernova remnants. AIP, 2001. http://dx.doi.org/10.1063/1.1377080.
Pełny tekst źródłaKrumholz, Mark R., Eduardo Telles, Renato Dupke i Daniela Lazzaro. "Star Formation in Molecular Clouds". W XV SPECIAL COURSES AT THE NATIONAL OBSERVATORY OF RIO DE JANEIRO. AIP, 2011. http://dx.doi.org/10.1063/1.3636038.
Pełny tekst źródłaStrong, Andy, Clive Dickinson i Eric Murphy. "Synchrotron emission from molecular clouds". W Cosmic Rays and the InterStellar Medium. Trieste, Italy: Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.221.0036.
Pełny tekst źródłaKlessen, Ralf S. "Fragmentation of molecular clouds with GRAPESPH". W The seventh astrophysical conference: Star formation, near and far. AIP, 1997. http://dx.doi.org/10.1063/1.52778.
Pełny tekst źródłaRaporty organizacyjne na temat "Molecular clouds"
Torres, D. High-Latitude Molecular Clouds as Gamma-Ray Sources for GLAST. Office of Scientific and Technical Information (OSTI), styczeń 2005. http://dx.doi.org/10.2172/839757.
Pełny tekst źródłaDigel, S. Small Molecular Clouds at High Latitudes as Gamma-Ray Sources for GLAST. Office of Scientific and Technical Information (OSTI), marzec 2005. http://dx.doi.org/10.2172/839933.
Pełny tekst źródłaLow, Mordecai-Mark Mac, Jayashree Toraskar, Jeffrey S. Oishi i Tom Abel. Dynamical Expansion of HII Regions From Ultracompact to Compact Sizes in Turbulent, Self-Gravitating Molecular Clouds. Office of Scientific and Technical Information (OSTI), maj 2006. http://dx.doi.org/10.2172/882832.
Pełny tekst źródłaKing, P. K. Gas Dynamics Near and Far: Observational Magnetohydrodynamics of Interstellar Molecular Clouds and X-Ray Ablation of Asteroids for the Earth's Defense. Office of Scientific and Technical Information (OSTI), czerwiec 2019. http://dx.doi.org/10.2172/1544929.
Pełny tekst źródłaShomer, Ilan, Louise Wicker, Uzi Merin i William L. Kerr. Interactions of Cloud Proteins, Pectins and Pectinesterases in Flocculation of Citrus Cloud. United States Department of Agriculture, luty 2002. http://dx.doi.org/10.32747/2002.7580669.bard.
Pełny tekst źródłaBacharach, Eran, i Sagar Goyal. Generation of Avian Pneumovirus Modified Clones for the Development of Attenuated Vaccines. United States Department of Agriculture, listopad 2008. http://dx.doi.org/10.32747/2008.7696541.bard.
Pełny tekst źródłaOffner, S., M. Krumholz, R. Klein i C. McKee. The Kinematics of Molecular Cloud Cores in the Presence of Driven and Decaying Turbulence: Comparisons with Observations. Office of Scientific and Technical Information (OSTI), kwiecień 2008. http://dx.doi.org/10.2172/938508.
Pełny tekst źródłaBanai, Menachem, i Gary Splitter. Molecular Characterization and Function of Brucella Immunodominant Proteins. United States Department of Agriculture, lipiec 1993. http://dx.doi.org/10.32747/1993.7568100.bard.
Pełny tekst źródłaNewton, Ronald, Joseph Riov i John Cairney. Isolation and Functional Analysis of Drought-Induced Genes in Pinus. United States Department of Agriculture, wrzesień 1993. http://dx.doi.org/10.32747/1993.7568752.bard.
Pełny tekst źródłaSadka, Avi, Mikeal L. Roose i Yair Erner. Molecular Genetic Analysis of Citric Acid Accumulation in Citrus Fruit. United States Department of Agriculture, marzec 2001. http://dx.doi.org/10.32747/2001.7573071.bard.
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