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
1. Verfasser: Hogan, Craig J.
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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.
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ispartof Astrophys. J.; (United States), 1987-05, Vol.316 (2), p.L59-L61
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source NASA Technical Reports Server; Alma/SFX Local Collection
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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