Bibliografías temáticas / Interstellar matter

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Literatura académica sobre el tema "Interstellar matter"

Autor: Grafiati
Publicado: 4 de junio de 2021
Última modificación: 29 de julio de 2024

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Artículos de revistas sobre el tema "Interstellar matter"

1

Lequeux, J., J. S. Mathis, K. S. de Boer, S. D’Odorico, B. G. Elmegreen, D. Flower, H. Habing, et al. "34. Interstellar Matter (Matiere Interstellaire)." Transactions of the International Astronomical Union 20, no. 01 (1988): 423–71. http://dx.doi.org/10.1017/s0251107x0000732x.

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The previous report started with optimistic remarks about the increasing importance of the study of interstellar matter in astronomy. This trend has largely been confirmed in the 1985-87 period and it is clear that the subject of our Commission is one of the most active fields of astronomical research. This is also shown by the rapidly growing number of members and by the constitution of new working groups. The major new event in the period has undoubtly been the availability of IRAS data.
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Habing, H. J., E. Falgarone, D. Flower, P. G. Martin, M. R. Rosa, T. Lozinskaya, and M. Dopita. "34 Interstellar Matter: Matiere Interstellaire." Transactions of the International Astronomical Union 22, no. 1 (1994): 367–97. http://dx.doi.org/10.1017/s0251107x00008117.

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Dopita, Michael A., Rafael Bachiller, Michael Burton, John Dyson, Debra Elmegreen, Thomas Henning, Sun Kwok, et al. "Division VI: Interstellar Matter: (Matière Interstellaire)." Transactions of the International Astronomical Union 24, no. 1 (2000): 277–80. http://dx.doi.org/10.1017/s0251107x00003175.

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Division VI of the International Astronomical Union deals with Interstellar Matter, and incorporates Commission 34. It gathers astronomers studying the diffuse matter in space between the stars, ranging from primordial intergalactic clouds via dust and neutral and ionised gas in galaxies to the densest molecular clouds and the processes by which stars are formed. There are approximately 730 members. The working groups in Planetary Nebulae and Cosmochemistry have served us well in organising periodic seminars in these subject areas. However, the Organising Committee has recognised that other de
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Reipurth, Bo. "Division VI: Interstellar Matter (Matiere Interstellaire)." Transactions of the International Astronomical Union 25, no. 2 (2007): 157–58. http://dx.doi.org/10.1017/s0251107x00026729.

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Reipurth, Bo, Rafael Bachiller, John Dyson, José Franco, Thomas Henning, Trung Hua, Sun Kwok, et al. "Division VI: Interstellar Matter: (Matiere Interstellaire)." Transactions of the International Astronomical Union 25, no. 1 (2002): 283–86. http://dx.doi.org/10.1017/s0251107x00001577.

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Bochkarev, Nikolai G. "Local interstellar matter and interstellar bubbles." Astronomical & Astrophysical Transactions 3, no. 1 (November 1992): 3–16. http://dx.doi.org/10.1080/10556799208230534.

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Peimbert, M., J. Lequeux, S. D’Odorico, B. G. Elmegreen, E. B. Kostyakova, J. S. Mathis, U. Mebold, et al. "34. Interstellar Matter." Transactions of the International Astronomical Union 19, no. 1 (1985): 437–78. http://dx.doi.org/10.1017/s0251107x00006532.

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It has become more evident during the last three years that the study of interstellar matter is paramount to understand the evolution of the universe and its constituents. From observations of the present state of the interstellar medium, in our galaxy, in other galaxies, and between galaxies, it is possible to test theories of: evolution of the universe, formation and evolution of galaxies, formation and evolution of stars and of the evolution of the interstellar medium itself. The amount of information on the interstellar medium that has been gathered during the 1982-1984 period has been ver
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Dyson, John, Thomas J. Millar, Bo Reipurth, You-Hua Chu, Gary J. Ferland, José Franco, Chon Trung Hua, et al. "DIVISION VI: INTERSTELLAR MATTER." Proceedings of the International Astronomical Union 3, T26B (December 2007): 173. http://dx.doi.org/10.1017/s1743921308023971.

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Division VI gathers astronomers studying the diffuse matter in space between stars, ranging from primordial intergalactic clouds, via dust and neutral and ionized gas in galaxies, to the densest molecular clouds and the processes by which stars are formed.
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Millar, Thomas J., You Hua Chu, John E. Dyson, Dieter Breitschwerdt, Michael G. Burton, Sylvie Cabrit, Paola Caselli, et al. "DIVISION VI: INTERSTELLAR MATTER." Proceedings of the International Astronomical Union 4, T27A (December 2008): 267–72. http://dx.doi.org/10.1017/s1743921308025659.

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Dyson, John, Tom Millar, You-Hua Chu, Gary Ferland, Pepe Franco, Trung Hua, Susana Lizano, et al. "Division VI: Interstellar Matter." Proceedings of the International Astronomical Union 1, T26A (December 2005): 267–71. http://dx.doi.org/10.1017/s1743921306004662.

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Commission 34 covers diffuse matter in space on scales ranging from the circumstellar to the galactic and intergalactic. As such it has enormous scope and because of this, it alone forms Division VI. Key aspects include star formation, matter around evolved stars, astrochemistry, nebulae, galactic and intergalactic clouds and the multitude of effects of the interaction of stars with their surroundings. Associated with these areas are a huge range of physical and chemical processes including hydrodynamics and magnetohydrodynamics, radiative processes, molecular physics and chemistry, plasma pro
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Tesis sobre el tema "Interstellar matter"

1

Hopwood, Madelaine E. L. "Interstellar matter in globular clusters." Thesis, Keele University, 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.323681.

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Danforth, Charles Weston. "Interstellar matter kinematics in the magellanic clouds." Available to US Hopkins community, 2003. http://wwwlib.umi.com/dissertations/dlnow/3080648.

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Hurst, Mark Edward. "Observational studies of stellar, circumstellar and interstellar matter." Thesis, University of Nottingham, 1999. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.312198.

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Kristen, Helmuth. "Dynamics of the interstellar matter in galaxies : isolated barred spiral galaxies : cloud formation processes /." Stockholm : Univ, 1998. http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&doc_number=008210174&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA.

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Malawi, Abdulrahman Ali. "Atomic hydrogen associated with high latitude IRAS cirrus clouds." Thesis, University of Manchester, 1989. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.664465.

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Roser, Joseph E. Vidali Gianfranco. "Laboratory simulations of chemical reactions on dust grains in the interstellar medium." Related electronic resource: Current Research at SU : database of SU dissertations, recent titles available full text, 2004. http://wwwlib.umi.com/cr/syr/main.

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Smith, Keith T. "Studies of interstellar matter on scales from 10AU to 10 kpc." Thesis, University of Nottingham, 2010. http://eprints.nottingham.ac.uk/12504/.

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This thesis presents four optical spectroscopic studies of absorption by matter in the diffuse interstellar medium on scales ranging from 10 AU to 10 kpc. The observations investigate two current problems in interstellar medium (ISM) research: small-scale structure (SSS), and the diffuse interstellar bands (DIBs). Very high spectral resolution observations of interstellar Na I, Ca I, Ca II, K I and CH absorption towards kappa Vel are presented. Combined with observations over the last 15 years taken from the literature, the small-scale structure in front of this star is probed on scales of ~ 1
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van, Dishoeck E. F. "Interstellar C2, CH, and CN in Translucent Molecular Clouds." Steward Observatory, The University of Arizona (Tucson, Arizona), 1988. http://hdl.handle.net/10150/623918.

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Optical absorption line techniques have been applied to the study of a number of translucent molecular clouds in which the total column densities are large enough that substantial molecular abundances can be maintained. Results are presented for a survey of absorption lines of interstellar C2, CH, and CN. Detections of CN through the A2II -X2E+ (1,0) and (2,0) bands of the red system are reported, and are compared with observations of the blue system for one line of sight. The population distributions in C2 provide diagnostic information on temperature and density. The measured column de
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9

Walker, Constance Elaine. "A submillimeter-millimeterwave study of the molecular gas in the nuclear regions of three nearby starburst galaxies." Diss., The University of Arizona, 1991. http://hdl.handle.net/10150/185738.

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In this thesis we use multi-transitional millimeter/submillimeter-wave molecular spectroscopy of CO and CS to determine the state of the molecular gas in the central regions of three starbursts: M82, IC342, and M83. High angular resolution 60 and 100 μm IRAS images provide complementary information about the thermal dust emission in IC342 and M83. Our CO observations reveal the presence of a molecular ring and supernovae driven wind in M82. In IC342 and M83 there is evidence for molecular bars and central rotating cores. The CO and CS line ratio analyses suggest a multicomponenet medium with c
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Porayko, Nataliya Konstantinovna [Verfasser]. "Probing the Interstellar Medium and Dark Matter with Pulsars / Nataliya Konstantinovna Porayko." Bonn : Universitäts- und Landesbibliothek Bonn, 2020. http://d-nb.info/1207923710/34.

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Libros sobre el tema "Interstellar matter"

1

Spitzer, Lyman. Physical processes in the interstellar medium. New York: Wiley, 1998.

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2

Voigt, H. H., ed. Interstellar Matter, Galaxy, Universe. Berlin/Heidelberg: Springer-Verlag, 1999. http://dx.doi.org/10.1007/b46102.

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1936-, Winnewisser G. (Gisbert), and SpringerLink (Online service), eds. Interstellar Molecules: Their Laboratory and Interstellar Habitat. Berlin, Heidelberg: Springer-Verlag Berlin Heidelberg, 2011.

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David, Skillman Evan, and University of Minnesota, eds. The Minnesota lectures on extragalactic neutral hydrogen: A series of lectures presented at the University of Minnesota, Minneapolis, Minnesota, from 27 March 1994 [i.e. 1995] to 2 June 1994 [i.e. 1995]. San Francisco, Calif: Astronomical Society of the Pacific, 1996.

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1974-, Haverkorn M., and Goss W. M, eds. SINS--small ionized and neutral structures in the diffuse interstellar medium: Proceedings of a workshop held at the National Radio Astronomy Observatory, Socorro, New Mexico, USA, 21-24 May 2006. San Francisco: Astronomical Society of the Pacific, 2007.

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McComas, David J. Interstellar Boundary Explorer (IBEX). Dordrecht: Springer, 2010.

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7

Kim, Dong-Woo, and Silvia Pellegrini, eds. Hot Interstellar Matter in Elliptical Galaxies. New York, NY: Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4614-0580-1.

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International Astronomical Union. General Assembly, ed. Hot interstellar matter in elliptical galaxies. Heidelberg: Springer, 2011.

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Meeting, Royal Society (Great Britain) Discussion. Material content of the universe: Proceedings of a Royal Society Discussion Meeting held on 23 and 24 October 1985. London: Royal Society, 1987.

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1944-, Ikeuchi S., and United States. National Aeronautics and Space Administration., eds. The disk-halo connection and the nature of the interstellar medium. Baltimore, MD: Space Telescope Science Institute, 1990.

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Capítulos de libros sobre el tema "Interstellar matter"

1

Flower, D. R., M. A. Dopita, F. C. Bruhweiler, M. G. Burton, D. M. Elmegreen, E. Falgarone, T. A. Lozinskaya, et al. "Interstellar Matter Matiere Interstellaire." In Reports on Astronomy, 397–414. Dordrecht: Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5762-9_33.

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McNally, Derek. "Interstellar Matter (Matiere Interstellaire)." In Reports on Astronomy, 373–420. Dordrecht: Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-011-3364-7_24.

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Lequeux, J., J. S. Mathis, K. S. de Boer, S. D’Odorico, B. G. Elmegreen, D. Flower, H. Habing, et al. "Interstellar Matter." In Reports on Astronomy, 423–71. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2981-4_25.

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Habing, H. J., E. Falgarone, D. Flower, M. R. Rosa, T. Lozinskaya, and M. Dopita. "Interstellar Matter." In Reports on Astronomy, 367–97. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1100-3_25.

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West, Richard M. "Interstellar Matter." In Reports on Astronomy, 437–78. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5392-5_25.

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Sofue, Yoshiaki. "Interstellar Matter." In Galactic Radio Astronomy, 33–56. Singapore: Springer Singapore, 2017. http://dx.doi.org/10.1007/978-981-10-3445-9_2.

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Hanslmeier, Arnold. "Interstellar Matter." In Introduction to Astronomy and Astrophysics, 463–78. Berlin, Heidelberg: Springer Berlin Heidelberg, 2022. http://dx.doi.org/10.1007/978-3-662-64637-3_12.

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Verschuur, Gerrit L. "An Extraterrestrial Matter." In Interstellar Matters, 290–302. New York, NY: Springer New York, 1989. http://dx.doi.org/10.1007/978-1-4612-4522-3_24.

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Verschuur, Gerrit L. "Molecules and Interstellar Matter." In Interstellar Matters, 234–47. New York, NY: Springer New York, 1989. http://dx.doi.org/10.1007/978-1-4612-4522-3_20.

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Verschuur, Gerrit L. "A Mysterious Interstellar Matter." In Interstellar Matters, 280–89. New York, NY: Springer New York, 1989. http://dx.doi.org/10.1007/978-1-4612-4522-3_23.

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Actas de conferencias sobre el tema "Interstellar matter"

1

Blades, J. C., and N. Panagia. "Interstellar abundances towards SN1987A." In Cosmic abundances of matter. AIP, 1989. http://dx.doi.org/10.1063/1.38015.

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Hovestadt, Dietrich, and Eberhard Möbius. "Interstellar neutrals in interplanetary space." In Cosmic abundances of matter. AIP, 1989. http://dx.doi.org/10.1063/1.38004.

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Meyer, Jean-Paul. "Elemental abundances in the interstellar medium ... and elsewhere." In Cosmic abundances of matter. AIP, 1989. http://dx.doi.org/10.1063/1.37991.

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Sahu, Kailash C., S. R. Pottasch, and Meenakshi Sahu. "Primordial lithium abundance from interstellar lithium lines towards SN 1987A." In Cosmic abundances of matter. AIP, 1989. http://dx.doi.org/10.1063/1.37984.

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Iacob, F. "ELECTRON-MOLECULAR CATION COLLISIONS IN INTERSTELLAR SPACE." In VI Conference on Active Galactic Nuclei and ravitational Lensing. Astronomical Observatory Belgrade, Volgina 7, 11060 Belgrade 38, Serbia, 2024. http://dx.doi.org/10.69646/aob24007.

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In the interstellar medium, highly excited states of molecules can form a state of matter called Rydberg Matter. Mainly, they are formed by the promotion of an electron from the lower layers of the molecule to the highly excited ones. However, these can also be formed by temporarily capturing an electron in high energy orbitals following its collisions with cations. This paper focuses on the latter, the collisional approach, which is more suitable for explaining these highly excited states that can be found in this environment. It should be mentioned that in this environment cations are abunda
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Moniez, Marc. "Searching for Galactic Hidden Gas through interstellar scintillation: The OSER project." In Identification of dark matter 2008. Trieste, Italy: Sissa Medialab, 2009. http://dx.doi.org/10.22323/1.064.0097.

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Green, James C., Patrick Jelinsky, and Stuart Bowyer. "The ratio of neutral helium to neutral hydrogen in the local interstellar medium." In Cosmic abundances of matter. AIP, 1989. http://dx.doi.org/10.1063/1.37979.

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Kajino, Fumiyoshi, Shinsuke Abe, Mizuho Arahori, Dario Barghini, Mario Edoardo Bertaina, Marco Casolino, Alberto Cellino, et al. "DIMS Experiment for Dark Matter and Interstellar Meteoroid Study." In 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0554.

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Soutoul, A., and P. Ferrando. "Propagation of cosmic-rays nuclei in the interstellar medium: The importance of energy losses revisited." In Cosmic abundances of matter. AIP, 1989. http://dx.doi.org/10.1063/1.37975.

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Kajino, Fumiyoshi. "DIMS Experiment for Macroscopic Dark Matter and Interstellar Meteoroid Study." In 38th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2023. http://dx.doi.org/10.22323/1.444.1376.

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Informes sobre el tema "Interstellar matter"

1

Wells, James D. Illuminating dark matter and primordial black holes with an interstellar antiproton spectrometer. Office of Scientific and Technical Information (OSTI), November 1998. http://dx.doi.org/10.2172/9903.

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