Littérature scientifique sur le sujet « Interstellar Atmosphere Chemistry »
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Articles de revues sur le sujet "Interstellar Atmosphere Chemistry"
Phillips, T. G., Ewine F. Van Dishoeck et Jocelyn B. Keene. « Interstellar H3O+ ». Symposium - International Astronomical Union 150 (1992) : 191–92. http://dx.doi.org/10.1017/s0074180900089993.
Texte intégralPeacock, Sarah, Travis S. Barman, Adam C. Schneider, Michaela Leung, Edward W. Schwieterman, Evgenya L. Shkolnik et R. O. Parke Loyd. « Accurate Modeling of Lyα Profiles and Their Impact on Photolysis of Terrestrial Planet Atmospheres ». Astrophysical Journal 933, no 2 (1 juillet 2022) : 235. http://dx.doi.org/10.3847/1538-4357/ac77f2.
Texte intégralBarnett, NeilW. « Spectroscopy of the Earth's Atmosphere and Interstellar Medium ». Analytica Chimica Acta 284, no 1 (décembre 1993) : 241. http://dx.doi.org/10.1016/0003-2670(93)80030-o.
Texte intégralWillacy, Karen, SiHe Chen, Danica J. Adams et Yuk L. Yung. « Vertical Distribution of Cyclopropenylidene and Propadiene in the Atmosphere of Titan ». Astrophysical Journal 933, no 2 (1 juillet 2022) : 230. http://dx.doi.org/10.3847/1538-4357/ac6b9d.
Texte intégralSmith, David, et Patrik Spanel. « Ions in the terrestrial atmosphere and in interstellar clouds ». Mass Spectrometry Reviews 14, no 4-5 (juillet 1995) : 255–78. http://dx.doi.org/10.1002/mas.1280140403.
Texte intégralRimmer, Paul B., Catherine Walsh et Christiane Helling. « Cosmic Rays, UV Photons, and Haze Formation in the Upper Atmospheres of Hot Jupiters ». Proceedings of the International Astronomical Union 8, S299 (juin 2013) : 303–4. http://dx.doi.org/10.1017/s1743921313008703.
Texte intégralMalmqvist, Per-Åke. « The RASSCF, RASSI, and CASPT2 Methods Used on Small Molecules of Astrophysical Interest ». International Astronomical Union Colloquium 146 (1994) : 338–52. http://dx.doi.org/10.1017/s0252921100021448.
Texte intégralNotsu, Shota, Christian Eistrup, Catherine Walsh et Hideko Nomura. « The composition of hot Jupiter atmospheres assembled within chemically evolved protoplanetary discs ». Monthly Notices of the Royal Astronomical Society 499, no 2 (25 septembre 2020) : 2229–44. http://dx.doi.org/10.1093/mnras/staa2944.
Texte intégralBergin, Edwin A., Geoffrey A. Blake, Fred Ciesla, Marc M. Hirschmann et Jie Li. « Tracing the ingredients for a habitable earth from interstellar space through planet formation ». Proceedings of the National Academy of Sciences 112, no 29 (6 juillet 2015) : 8965–70. http://dx.doi.org/10.1073/pnas.1500954112.
Texte intégralWang, Zhe-Chen, Callie A. Cole, Nicholas J. Demarais, Theodore P. Snow et Veronica M. Bierbaum. « Reactions of Azine Anions with Nitrogen and Oxygen Atoms : Implications for Titan’s Upper Atmosphere and Interstellar Chemistry ». Journal of the American Chemical Society 137, no 33 (17 août 2015) : 10700–10709. http://dx.doi.org/10.1021/jacs.5b06089.
Texte intégralThèses sur le sujet "Interstellar Atmosphere Chemistry"
Jamal, Eddine Nour. « Reactivity of molecular anions at low temperature : implications for the chemistry of the interstellar medium ant Titan's atmosphere ». Thesis, Rennes 1, 2017. http://www.theses.fr/2017REN1S132/document.
Texte intégralEver since their discovery in various astrophysical environments, polyyne anions CxH¯ (x = 2, 4, 6) and cyanopolyyne anions CxN¯ (x = 1, 3, 5) have received a considerable attention. These anions appear to be playing important roles in their environments. However, low temperature data on the chemical pathways leading to their formation and destruction is still scarce, especially regarding product identity and branching ratios. To address this issue, we have engaged in the investigation of the reactivity of these molecular anions by employing dedicated instruments coupling subsonic and supersonic flows with mass spectrometry methods. In this fashion, we have investigated the reactivity of C3N¯ anions with cyanoacetylene (HC3N) as well as the reactivity of CN¯, C3N¯, and C5N¯ with formic acid (HCOOH) from 298 K down to temperatures as low as 36 K. We report in this work the rate coefficient, the nature of the products, and the branching ratios of these reactions.This work also addresses the prototype selected ion source in our laboratory, which was recently implemented in order to extend our investigation to other anions of astrophysical interest (e.g. CxH¯ and Cx¯ anions). A description of this instrument as well as some preliminary results are presented in this work. This thesis, «Reactivity of Molecular Anions at Low Temperature: Implications for the Chemistry of the Interstellar medium and Titan’s atmosphere», was carried out at the Institut de Physique de Rennes and the Ecole Nationale Supérieure de Chimie de Rennes.Keywords: astrochemistry, Titan’s atmosphere, molecular anions, gas phase kinetics, supersonic flow, mass spectrometry, selected ion source
Landera, Alexander. « Formation of Polycyclic Aromatic Hydrocarbons and Nitrogen Containing Polcyclic Aromatic Compounds in Titan's Atmosphere, the Interstellar Medium and Combustion ». FIU Digital Commons, 2013. http://digitalcommons.fiu.edu/etd/991.
Texte intégralBlanksby, Stephen J. « "Gas phase synthesis of interstellar cumulenes : mass spectrometric and theoretical studies" / ». Title page, contents and summary only, 1999. http://web4.library.adelaide.edu.au/theses/09PH/09phb6423.pdf.
Texte intégralCopies of author's previously published articles inserted. Supplement entitled: Addressing referee concerns, stapled to back end paper (5 leaves). Bibliography: leaves 199-212.
Vásquez, Mencos Abraham Alejandro. « The Nitrogen Chemistry in Solid Phase at Cryogenic Temperatures : Molecular Evolutions in Interstellar Clouds and Planetary Atmospheres ». Thesis, Sorbonne université, 2018. http://www.theses.fr/2018SORUS256.
Texte intégralNitrogen is the fifth most abundant element in the Universe, and the most significant reservoirs of this element are molecular clouds, dark clouds, and proto-planetary discs. Due to the conditions of the interstellar medium, most of the nitrogen exists in atomic form. Even the enormous abundance of this element there are not many studies aimed at understanding the role that nitrogen plays in the chemistry of dark molecular clouds and other cold regions of the Universe where the UV light and other energetic particles are not able to penetrate. In the present Ph-D thesis, we have explored the reactivity of atomic nitrogen in ground state N(4S) thermally induced with small organic compounds in the solid phase at cryogenic temperatures from 3 to 40K using Fourier Transform Infrared Spectroscopy (FTIR) analysis. We have shown that gradual heating in a first step, between 3 and 10K, stimulates N(4S) - N(4S) recombination and the consequent formation of the excited forms of nitrogen N2(A) and N(2D). These species play an essential role in the dissociation of H-C bearing species to form radicals. Then, in a second step, the continuous heating from 10 to 40K, induces the recombination of the radicals formed in the first step to produce more stable and complex compounds. During this process, there are observed reactions of addition, H-elimination, C-N, C-C formation, molecular fragmentation and isomerization. From these experiments, we have demonstrated that role of atomic nitrogen in dark molecular clouds is equivalent to that of UV light in diffuse clouds
Blanksby, Stephen J. (Stephen James). « "Gas phase synthesis of interstellar cumulenes : mass spectrometric and theoretical studies" / by Stephen J. Blanksby ». 1999. http://hdl.handle.net/2440/19402.
Texte intégralSupplement entitled: Addressing referee concerns, stapled to back end paper (5 leaves).
Bibliography: leaves 199-212.
xii, 212 leaaves : ill. ; 30 cm.
Title page, contents and abstract only. The complete thesis in print form is available from the University Library.
Presents methodologies for the synthesis of charged analogues of a number of molecular species residing in the large gas clouds which are present in regions of interstellar and circumstellar space. Quantum chemical calculations have been used to provide further insight into the structure and energetics of these molecules.
Thesis (Ph.D.)--University of Adelaide, Dept. of Chemistry, 1999
Blanksby, Stephen J. (Stephen James). « "Gas phase synthesis of interstellar cumulenes : mass spectrometric and theoretical studies" / by Stephen J. Blanksby ». Thesis, 1999. http://hdl.handle.net/2440/19402.
Texte intégralSupplement entitled: Addressing referee concerns, stapled to back end paper (5 leaves).
Bibliography: leaves 199-212.
xii, 212 leaaves : ill. ; 30 cm.
Presents methodologies for the synthesis of charged analogues of a number of molecular species residing in the large gas clouds which are present in regions of interstellar and circumstellar space. Quantum chemical calculations have been used to provide further insight into the structure and energetics of these molecules.
Thesis (Ph.D.)--University of Adelaide, Dept. of Chemistry, 1999
Livres sur le sujet "Interstellar Atmosphere Chemistry"
Krasnopolʹskiĭ, V. A. Photochemistry of Triton's atmosphere and ionosphere. [Washington, D.C : National Aeronautics and Space Administration, 1995.
Trouver le texte intégralKrasnopolʹskiĭ, V. A. Photochemistry of Triton's atmosphere and ionosphere. [Washington, D.C : National Aeronautics and Space Administration, 1995.
Trouver le texte intégralSymposium, COSPAR Scientific Commission F. F3 1. Life sciences : new insights into complex organics in space : Proceedings of the F3.1 Symposium of COSPAR Scientific Commission F which was held during the thirty-second COSPAR Scientific Assembly, Nagoya, Japan, 12-19 July, 1998. Oxford : Pergamon [for the] Committee on Space Research, 1999.
Trouver le texte intégralAssembly, COSPAR Scientific. Life sciences : Complex organics in space : proceedings of the F3.2 symposium of COSPAR Scientific Commission F which was held during the thirty-first COSPAR scientific assembly, Birmingham, U.K., 14-21 July 1996. Kidlington, Oxford : Published for the Committee on Space Research [by] Pergamon, 1997.
Trouver le texte intégralAssembly, COSPAR Scientific. Life sciences : Recent dosimetry results, chromosome damage and heritable effects : proceedings of the F2.6 and F2.9 symposia of COSPAR Scientific Commission F which was held during the thirty-first COSPAR Scientific Assembly, Birmingham, U.K., 14-21 July 1996. Kidlington, Oxford : Published for the Committee on Space Research [by] Pergamon, 1998.
Trouver le texte intégralM, Wheeler R., et COSPAR Scientific Commission F, dir. Life sciences : Life support system studies-I : proceedings of the F4.6, F4.8, F4.2 and F4.9 symposia of COSPAR Scientific Commission F which was held during the thirty-first COSPAR Scientific Assembly, Birmingham, U.K., 14-21 July 1996. Oxford, [England] : Published for the Committee on Space Research [by] Pergamon, 1997.
Trouver le texte intégralAssembly, COSPAR Scientific. Life sciences : Exobiology : proceedings of the F3.1, F3.3, F3.4 and F3.5 symposia of COSPAR Scientific Commission F which were held during the thirty-first COSPAR Scientific Assembly, Birmingham, U.K., 14-21 July 1996. Kidlington, Oxford : Published for the Committee on Space Research [by] Pergamon, 1998.
Trouver le texte intégralAssembly, COSPAR Scientific. Life sciences : Exobiology : proceedings of the F3.3 and F3.5 symposia of COSPAR Scientific Commission F which was held during the thirty-second COSPAR Scientific Assembly, Nagoya, Japan, 12-19 July, 1998. Oxford : Published for the Committee on Space Research [by] Pergamon, 1999.
Trouver le texte intégralAssembly, COSPAR Scientific. Life sciences : Space and Mars recent results : proceedings of the F3.1, F3.4, F2.4 and F3.8 Symposia of COSPAR Scientific Commission F, which were held during the Thirtieth COSPAR Scientific Assembly, Hamburg, Germany, 11-21 July, 1994. Oxford, UK : Published for the Committee on Space Research [by] Pergamon, 1996.
Trouver le texte intégralAssembly, COSPAR Scientific. Life sciences : Space flight and the central nervous system : the potential independent and synergistic effects of microgravity and radiation : proceedings of the F2.4 Symposium of COSPAR Scientific Commission F which was held during the Thirty-first COSPAR Scientific Assembly, Birmingham, U.K., 14-21 July 1996. Oxford : Published for the Committee on Space Research [by] Pergamon, 1998.
Trouver le texte intégralChapitres de livres sur le sujet "Interstellar Atmosphere Chemistry"
Zalasiewicz, Jan. « 100 Million Years AD ». Dans The Earth After Us. Oxford University Press, 2008. http://dx.doi.org/10.1093/oso/9780199214976.003.0007.
Texte intégralIRVINE, W. M., et R. F. KNACKE. « THE CHEMISTRY OF INTERSTELLAR GAS AND GRAINS ». Dans Origin and Evolution of Planetary and Satellite Atmospheres, 3–34. University of Arizona Press, 1989. http://dx.doi.org/10.2307/j.ctv20dsb5m.5.
Texte intégralActes de conférences sur le sujet "Interstellar Atmosphere Chemistry"
KLEMPERER, WILLIAM. « SOME THOUGHTS ON INTERSTELLAR CHEMISTRY ». Dans Contributions to Atomic, Molecular, and Optical Physics, Astrophysics, and Atmospheric Physics. PUBLISHED BY IMPERIAL COLLEGE PRESS AND DISTRIBUTED BY WORLD SCIENTIFIC PUBLISHING CO., 2009. http://dx.doi.org/10.1142/9781848164703_0006.
Texte intégralTHADDEUS, PATRICK. « STILL MORE THOUGHTS ON INTERSTELLAR CHEMISTRY ». Dans Contributions to Atomic, Molecular, and Optical Physics, Astrophysics, and Atmospheric Physics. PUBLISHED BY IMPERIAL COLLEGE PRESS AND DISTRIBUTED BY WORLD SCIENTIFIC PUBLISHING CO., 2009. http://dx.doi.org/10.1142/9781848164703_0011.
Texte intégralHARTQUIST, T. W., S. VAN LOO et S. A. E. G. FALLE. « HOW INTERSTELLAR CHEMISTRY (AND ASTROCHEMISTRY MORE GENERALLY) BECAME USEFUL ». Dans Contributions to Atomic, Molecular, and Optical Physics, Astrophysics, and Atmospheric Physics. PUBLISHED BY IMPERIAL COLLEGE PRESS AND DISTRIBUTED BY WORLD SCIENTIFIC PUBLISHING CO., 2009. http://dx.doi.org/10.1142/9781848164703_0012.
Texte intégralMorin, P. « Free Electron Laser Induced Dissociation of Molecules Probed with Synchrotron Radiation ». Dans Free-Electron Laser Applications in the Ultraviolet. Washington, D.C. : Optica Publishing Group, 1988. http://dx.doi.org/10.1364/fel.1988.wc2.
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