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THE STRUCTURE AND KINEMATICS OF THE CIRCUMGALACTIC MEDIUM FROM FAR-ULTRAVIOLET SPECTRA OF z ~ 2-3 GALAXIES

Author
STEIDEL, Charles C1 ; ERB, Dawn K2 ; SHAPLEY, Alice E3 ; PETTINI, Max4 5 ; REDDY, Naveen6 ; BOGOSAVLJEVIC, Milan1 ; RUDIE, Gwen C1 ; RAKIC, Olivera7
[1] California Institute of Technology, MS 249-17, Pasadena, CA 91125, United States
[2] Department of Physics, University of California Santa Barbara, Santa Barbara, CA 93106, United States
[3] Department of Physics and Astronomy, University of California Los Angeles, 430 Portola Plaza, Box 951547, Los Angeles, CA 90095, United States
[4] Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, United Kingdom
[5] International Centre for Radio Astronomy Research, University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia
[6] National Optical Astronomy Observatories, 950 North Cherry Avenue, Tucson, AZ 85258, United States
[7] Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden, Netherlands
Source

The Astrophysical journal. 2010, Vol 717, Num 1, pp 289-322, 34 p ; 1 ; ref : 1 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
IOP, Bristol
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
cosmology: observations galaxies: evolution galaxies: high-redshift
Keyword (fr)
Cinématique Cosmologie Déplacement vers le rouge Evolution galaxies Galaxies Spectre UV
Keyword (en)
Kinematics Cosmology Red shift Galaxy evolution Galaxies Ultraviolet spectra
Keyword (es)
Evolución galaxias
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
22973754

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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