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On the nature of the heat source for damped Lyα systems

Author
WOLFE, Arthur M1 ; HOWK, J. Christopher1 ; GAWISER, Eric2 ; PROCHASKA, Jason X3 ; LOPEZ, Sebastian4
[1] Department of Physics and Center for Astrophysics and Space Sciences, University of California at San Diego, Code 0424, 9500 Gilman Drive, La Jolla, CA 92093, United States
[2] Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101, United States
[3] University of California Observatories/Lick Observatory, University of California, 373 Interdisciplinary Sciences, Santa Cruz, CA 95464, Chile
[4] Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Las Condes, Santiago, Chile
Source

The Astrophysical journal. 2004, Vol 615, Num 2, pp 625-644, 20 p ; 1 ; ref : 43 ref

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Gaz neutre Quasar Raie absorption Source chaleur Evolution galaxies
Keyword (en)
Neutral gas Quasars Absorption line Heat sources Galaxy evolution
Keyword (es)
Gas neutro Raya absorción
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D54 Quasars. Active or peculiar galaxies, objects, and systems / 001E03D54A Quasars

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16358955

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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