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Relevant bibliographies by topics / Interstellar and Intergalactic Matter

Academic literature on the topic 'Interstellar and Intergalactic Matter'

Author: Grafiati

Published: 10 December 2022

Last updated: 29 January 2023

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Journal articles on the topic "Interstellar and Intergalactic Matter"

1

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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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 processes and others too numerous to name. These are complemented by an equally huge range of observational studies using practically all space and ground-based instrumentation at nearly all observable wavelengths. A glance at any data-base of publications over the past few years attests to the vigorous state of these studies. The current membership of the Division is around 800. It also has three separate working groups.

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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 developing areas of the ISM are not properly represented in the current organisation. In January 1997, the Division formed a new ISM working group on Star Forming Regions including cross-divisional representation to monitor progress in their fields and to help develop proposals for future IAU Symposia or Colloquia. In the future, especially in view of the rapid developments in spaceborne X-ray and IR astronomy, Division VI also hopes to form other working groups on the Hot ISM and the Extragalactic ISM.

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Roos, M., S. Bowyer, M. Lampton, and J. T. Peltoniemi. "Do Massive Neutrinos Ionize Intergalactic HI?" Symposium - International Astronomical Union 168 (1996): 563–67. http://dx.doi.org/10.1017/s0074180900110708.

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The radiative decay of massive relic 30eV neutrinos could explain several observational puzzles including the missing dark matter in the universe and the anomalous degree of ionization of interstellar matter in the Galaxy. We note that various non-standard particle physics models with extended scalar sector or minimal supersymmetry have sufficient freedom to accommodate such neutrinos. We discuss observational constraints in the immediate Solar neighborhood, in nearby regions of low interstellar absorption, in the Galactic halo, in clusters of galaxies, and in extragalactic space. Although some observations have been interpreted as ruling out this picture, we note that this is true only for models in which extreme concentrations of neutrinos occur in clusters of galaxies. An instrument is under development to measure the cosmic diffuse EUV background in the local Solar neighborhood, for flight on the Spanish Minisat satellite platform. This instrument will have the capability of providing a definitive test of the radiative neutrino decay hypothesis.

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Taniguchi, Yoshiaki. "IAU Symposium No. 217 Recycling of Intergalactic and Interstellar Matter." TRENDS IN THE SCIENCES 9, no. 5 (2004): 76. http://dx.doi.org/10.5363/tits.9.5_76.

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Pettini, M. "AAT Observations of the Interstellar Medium towards SN 1987A." Publications of the Astronomical Society of Australia 7, no. 4 (1988): 527–34. http://dx.doi.org/10.1017/s1323358000022736.

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AbstractThe exceptional brightness of SN 1987A has provided a unique opportunity to probe intervening gas clouds in the disk and halo of our Galaxy and in the Large Magellanic Cloud, as well as intergalactic matter between the two. At the AAO we have exploited this opportunity in two ways: in searches for very weak interstellar features requiring exceptionally high signal-to-noise ratio spectra, and in recording known interstellar lines with unprecedentedly high spectral resolution. We are also monitoring photographically the evolution of the light-echoes to map the three-dimensional distribution of interstellar matter near the supernova. Surprisingly high column densities of million-degree gas have been found in the LMC through the first detection of [Fe X] in absorption. The hot gas may fill the interior of a ‘superbubble’, created by the combined effects of previous supernovae in this active region of star-formation; this cavity may be related to the shells of interstellar matter giving rise to the light-echoes. The ultra-high resolution observations, which required the rapid construction of a dedicated new spectrograph, were successful in resolving the hyperfine structure of the sodium D lines in several interstellar clouds. This implies that the clouds are at temperatures of at most 170 K and have internal turbulent velocities of no more than 0.3 km s−1, even though some are moving with high velocities relative to the Sun.

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Cashman, Frances H., Varsha P. Kulkarni, Romas Kisielius, Gary J. Ferland, and Pavel Bogdanovich. "Atomic Data Revisions for Transitions Relevant to Observations of Interstellar, Circumgalactic, and Intergalactic Matter." Astrophysical Journal Supplement Series 230, no. 1 (May 19, 2017): 8. http://dx.doi.org/10.3847/1538-4365/aa6d84.

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Shull, J. Michael. "Atomic data needs for studies of the interstellar and intergalactic medium." Physica Scripta T47 (January 1, 1993): 165–70. http://dx.doi.org/10.1088/0031-8949/1993/t47/026.

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Komiya, Yutaka, Takuma Suda, Asao Habe, and Masayuki Fujimoto. "Galactic archeology with extremely metal-poor stars." Proceedings of the International Astronomical Union 4, S255 (June 2008): 330–35. http://dx.doi.org/10.1017/s1743921308025027.

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AbstractExtremely metal-poor (EMP) stars are thought to be formed in the low-mass protogalaxies as building blocks of the Milky Way and can be probes to investigate the early stage of galaxy formation and star formation in the early universe. We study the formation history of EMP stars in the Milky Way halo using a new model of chemical evolution based on the hierarchical theory of the galaxy formation. We construct the merging history of the Milky Way halo based on the extended Press-Schechter formalism, and follow the star formation and chemical evolution along the merger tree. The abundance trends and number of low-mass stars predicted in our model are compared with those of observed EMP stars. Additionally, in order to clarify the origin of hyper metal poor stars, we investigate the change of the surface metal abundances of stars by accretion of interstellar matter. We also investigate the pre-enrichment of intergalactic matter by the first supernovae.

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Pettini, Max. "Studies of the ISM in the LMC using SN1987A." Symposium - International Astronomical Union 148 (1991): 431. http://dx.doi.org/10.1017/s0074180900201071.

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The exceptional brightness of SN1987A provided a wealth of opportunities for probing not only the interstellar medium in our Galaxy and in the Large Magellanic Cloud (LMC), but also any intergalactic matter between the two. Spectroscopic work has been directed both towards searches for very weak absorption lines, which require data of exceptionally high signal-to-noise ratio, and towards recording spectra of known features at unprecedentedly high resolution. Both approaches have yielded exciting and unexpected results. The first detection of [FeX] absorption has revealed the presence of million-degree gas in the interstellar medium of the LMC, possibly resulting from the explosions of previous supernovae in the 30-Doradus HII region. The ultra-high-resolution observations have been successful in resolving the hyperfine structure of the sodium D lines in several interstellar clouds along the line of sight to the supernova. This implies that the clouds are at temperatures of, at most, 170 K and have internal turbulent velocities of not more than 0.2 km s−1; large-scale motions thus appear to be mainly subsonic in these clouds. Radio observations of HI emission at 21-cm with the Parkes telescope have been combined with measurements of a variety of ultraviolet absorption lines, obtained with the International Ultraviolet Explorer satellite, to give the most detailed picture yet of the chemical composition of the gas between the Galaxy and the LMC. Finally, photographic monitoring of the light echo of SN 1987A over the last two years has provided a three-dimensional view of the interstellar environment in which SN 1987A exploded, complementing vividly the information deduced from the spectroscopic results.

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Dissertations / Theses on the topic "Interstellar and Intergalactic Matter"

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Kollmeier, Juna Ariele. "The intergalactic medium absorption, emission, disruption /." Columbus, Ohio : Ohio State University, 2006. http://rave.ohiolink.edu/etdc/view?acc%5Fnum=osu1153856075.

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Williams, Rik Jackson. "The warm-hot environment of the Milky Way." Columbus, Ohio : Ohio State University, 2006. http://rave.ohiolink.edu/etdc/view?acc%5Fnum=osu1154972702.

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Koay, Jun Yi. "Interstellar and intergalactic scattering as astrophysical probes." Thesis, Curtin University, 2012. http://hdl.handle.net/20.500.11937/2364.

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The scattering of radio waves and multipath propagation in the interstellar medium (ISM) of our Galaxy produces various observable phenomena such as the interstellar scintillation (ISS) and angular broadening of compact radio sources, as well as the temporal smearing of impulsive radio bursts. These effects have been harnessed as probes of the ISM and of the background sources themselves. On the other hand, scattering in the intergalactic medium (IGM) has yet to be incontrovertibly detected, and is a main target of future surveys and instruments, since the IGM constitutes the main reservoir of baryons in the Universe. The first part of this thesis makes use of observational data from a survey of interstellar scintillation (ISS) of compact Active Galactic Nuclei (AGNs) to further investigate the nature of these sources, the ISM, ISS, and methods of handling variability data in the presence of stochastic and systematic errors. This study therefore acts as a technical and scientific demonstrator for future large-scale surveys of ISS and the variable radio sky.The results of this study further strengthen the link between AGN variability at radio wavelengths with ISS, and show how the spectral indices and mean flux densities of the sources, as well as observing frequencies, all influence the observed ISS characteristics. Six new rapid scintillators with characteristic time-scales of . 2 hours were identified in the sample, providing new insight into the origin of rapid and extreme scintillation. This thesis also presents the first detailed investigation into the origin of the suppresion of ISS for AGNs at z & 2 as discovered by the Micro-Arcsecond Scintillation Induced Variability (MASIV) Survey, a precursor to the present work. I determined that the redshift dependence of ISS is partially linked to the steepening of source spectral indices (_8.4 4.9) with redshift, caused either by selection biases or AGN evolution, coupled with weaker ISS in the _8.4 4.9 < −0.4 sources. Selecting only the −0.4 < _8.4 4.9 < 0.4 sources, the redshift dependence of ISS is still significant, but is not significantly steeper than the expected (1 + z)0.5 scaling of source angular sizes due to cosmological expansion for a brightness temperature and flux-limited sample of sources. No significant evidence of scatter broadening in the IGM was found, placing the strongest upper limit to date of . 8μas at 4.9 GHz for sight-lines to the most compact, _ 10μas sources.The second part of the thesis makes use of this observational limit on IGM scattering, together with extensions of ISM scattering models to cosmological scales, to investigate the detectability of the IGM with next generation radio arrays. While angular broadening in the IGM is insignificant for most sight-lines and appears difficult to resolve even with space VLBI, significant temporal smearing of extragalactic radio transients cannot be ruled out, and provides the best chance of detecting IGM scattering. However, the corresponding reduction in the signal-to-noise ratio of these bursts potentially places crippling limits on the detectability of such transient pulses in the first place, particularly at frequencies below _ 1 GHz. This has important ramifications for the optimization of observational strategies for detecting extragalactic radio transients with low-frequency instruments such as the Murchison Widefield Array (MWA), the Low Frequency Array (LOFAR) and the low frequency component of the Square Kilometre Array (SKA).

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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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Majeed, Qasim S. "Mid-infrared spectroscopy of solids in relation to the composition in interstellar and intergalactic dust." Thesis, Cardiff University, 1990. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.303977.

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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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Krakau, Steffen [Verfasser], Reinhard [Gutachter] Schlickeiser, and Horst [Gutachter] Fichtner. "Propagation of cosmic rays in the interstellar and intergalactic medium / Steffen Krakau ; Gutachter: Reinhard Schlickeiser, Horst Fichtner." Bochum : Ruhr-Universität Bochum, 2017. http://d-nb.info/1129452476/34.

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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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Books on the topic "Interstellar and Intergalactic Matter"

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Physics of the interstellar and intergalactic medium. Princeton: Princeton University Press, 2011.

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Symposium, International Astronomical Union. Recycling intergalactic and interstellar matter: Proceedings of the 217th symposium of the International Astronomical Union held during the IAU General Assembly XXV, Sydney, Australia, 14-17 July 2003. [San Francisco, Calif.]: Published on behalf of the IAU by Astronomical Society of the Pacific, 2004.

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Kennicutt, R. C. Galaxies: Interactions and induced star formation. Berlin: Springer, 1998.

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L, Sorochenko R., ed. Radio recombination lines: Their physics and astronomical applications. Dordrecht: Kluwer Academic Publishers, 2002.

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

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Interstellar medium: New research. Hauppauge, N.Y: Nova Science Publishers, 2011.

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

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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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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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Book chapters on the topic "Interstellar and Intergalactic Matter"

1

Dorfi, E. A. "Magnetic Braking of Interstellar Clouds." In Galactic and Intergalactic Magnetic Fields, 287–88. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0569-6_87.

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Moran, J. M. "Magnetic Fields in Interstellar Masers." In Galactic and Intergalactic Magnetic Fields, 301–3. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0569-6_91.

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Gisler, Galen. "Diamagnetic Cavities in the Interstellar Medium." In Galactic and Intergalactic Magnetic Fields, 168. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0569-6_50.

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Grabińska, T. "Intergalactic Dust Matter." In Astrophysics and Space Science Library, 357–58. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0903-8_42.

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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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Spangler, S. R. "Interstellar Magnetohydrodynamic Waves as Revealed by Radio Astronomy." In Galactic and Intergalactic Magnetic Fields, 176. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0569-6_52.

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Dolginov, A. Z. "Dust Grain Orientation in the Interstellar Magnetic Field." In Galactic and Intergalactic Magnetic Fields, 242–44. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0569-6_76.

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Conference papers on the topic "Interstellar and Intergalactic Matter"

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Kasdin, N. Jeremy, Tomonori Usuda, Motohide Tamura, and Miki Ishii. "THEIA: Telescope for Habitable Exoplanets and Interstellar∕Intergalactic Astronomy." In EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY: Proceedings of the International Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3215895.

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Richter, Philipp, Blair D. Savage, Todd M. Tripp, and Kenneth R. Sembach. "Baryons in the Warm-hot Intergalactic Medium." In Baryons in Dark Matter Halos. Trieste, Italy: Sissa Medialab, 2004. http://dx.doi.org/10.22323/1.014.0002.

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Mushotzky, Richard. "Abundances of the elements in the intergalactic medium." In Cosmic abundances of matter. AIP, 1989. http://dx.doi.org/10.1063/1.37994.

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Shapiro, Paul R., and Hugo Martel. "The effect of reionization of the intergalactic medium of galaxy formation." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48373.

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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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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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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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Reports on the topic "Interstellar and Intergalactic Matter"

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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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