On the physical state of QSO Lyman-alpha absorption clouds
Arguments are presented that QSO Lyman-alpha absorption lines might arise in denser environments than is usually thought, with a larger neutral fraction in the gas than in the usual models of rarefied intergalactic clouds, and a much smaller total mean mass density in Lyman-alpha clouds. A model is...
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Veröffentlicht in: | Astrophys. J.; (United States) 1987-05, Vol.316 (2), p.L59-L61 |
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container_title | Astrophys. J.; (United States) |
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creator | Hogan, Craig J. |
description | Arguments are presented that QSO Lyman-alpha absorption lines might arise in denser environments than is usually thought, with a larger neutral fraction in the gas than in the usual models of rarefied intergalactic clouds, and a much smaller total mean mass density in Lyman-alpha clouds. A model is sketched in which collapse or collision of thermally unstable protogalactic clouds forms shocks which trigger the collapse of cool thin sheets. The statistical properties of absorption lines formed in this way are consistent with those of the observed Lyman-alpha forest. |
doi_str_mv | 10.1086/184892 |
format | Article |
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A model is sketched in which collapse or collision of thermally unstable protogalactic clouds forms shocks which trigger the collapse of cool thin sheets. The statistical properties of absorption lines formed in this way are consistent with those of the observed Lyman-alpha forest.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1086/184892</identifier><identifier>CODEN: ASJOAB</identifier><language>eng</language><publisher>Legacy CDMS: University of Chicago Press</publisher><subject>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources ; ABSORPTION SPECTRA ; Astronomy ; Astrophysics ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; COSMIC GASES ; COSMIC RADIO SOURCES ; Earth, ocean, space ; Exact sciences and technology ; FLUIDS ; GASES ; GRAVITATIONAL COLLAPSE ; LYMAN LINES ; MASS ; QUASARS ; Quasars. Active or peculiar galaxies, objects, and systems ; SPECTRA ; Stellar systems. 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The statistical properties of absorption lines formed in this way are consistent with those of the observed Lyman-alpha forest.</description><subject>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources</subject><subject>ABSORPTION SPECTRA</subject><subject>Astronomy</subject><subject>Astrophysics</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>COSMIC GASES</subject><subject>COSMIC RADIO SOURCES</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>FLUIDS</subject><subject>GASES</subject><subject>GRAVITATIONAL COLLAPSE</subject><subject>LYMAN LINES</subject><subject>MASS</subject><subject>QUASARS</subject><subject>Quasars. Active or peculiar galaxies, objects, and systems</subject><subject>SPECTRA</subject><subject>Stellar systems. Galactic and extragalactic objects and systems. 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Active or peculiar galaxies, objects, and systems</topic><topic>SPECTRA</topic><topic>Stellar systems. Galactic and extragalactic objects and systems. The universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hogan, Craig J.</creatorcontrib><creatorcontrib>Steward Observatory, Tucson, AZ</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Astrophys. J.; (United States)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hogan, Craig J.</au><aucorp>Steward Observatory, Tucson, AZ</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>On the physical state of QSO Lyman-alpha absorption clouds</atitle><jtitle>Astrophys. J.; (United States)</jtitle><date>1987-05-15</date><risdate>1987</risdate><volume>316</volume><issue>2</issue><spage>L59</spage><epage>L61</epage><pages>L59-L61</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><coden>ASJOAB</coden><abstract>Arguments are presented that QSO Lyman-alpha absorption lines might arise in denser environments than is usually thought, with a larger neutral fraction in the gas than in the usual models of rarefied intergalactic clouds, and a much smaller total mean mass density in Lyman-alpha clouds. A model is sketched in which collapse or collision of thermally unstable protogalactic clouds forms shocks which trigger the collapse of cool thin sheets. The statistical properties of absorption lines formed in this way are consistent with those of the observed Lyman-alpha forest.</abstract><cop>Legacy CDMS</cop><pub>University of Chicago Press</pub><doi>10.1086/184892</doi></addata></record> |
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subjects | 640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources ABSORPTION SPECTRA Astronomy Astrophysics CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC GASES COSMIC RADIO SOURCES Earth, ocean, space Exact sciences and technology FLUIDS GASES GRAVITATIONAL COLLAPSE LYMAN LINES MASS QUASARS Quasars. Active or peculiar galaxies, objects, and systems SPECTRA Stellar systems. Galactic and extragalactic objects and systems. The universe |
title | On the physical state of QSO Lyman-alpha absorption clouds |
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