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Coincident, 100 kpc scale damped Lyα absorption towards a binary QSO : how large are galaxies at z ∼ 3?

Author
ELLISON, Sara L1 ; HENNAWI, Joseph F2 ; MARTIN, Crystal L3 ; SOMMER-LARSEN, Jesper4 5
[1] Department Physics & Astronomy, University of Victoria, 3800 Finnerty Road, Victoria, BC, V8P 1A1, Canada
[2] Department Physics & Astronomy, University of California, Berkeley, United States
[3] Department Physics & Astronomy, University of California, Santa Barbara, United States
[4] Dark Cosmology Centre, Niels Bohr Institute, Juliane Maries Vej 30, 2100 Copenhagen, Denmark
[5] Institute of Astronomy, University of Tokyo, Osawa 2-21-1, Mitaka, Tokyo 181-0015, Japan
Source

Monthly Notices of the Royal Astronomical Society. 2007, Vol 378, Num 3, pp 801-818, 18 p ; ref : 1 p.1/4

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Blackwell Science, Oxford
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
galaxies: abundances galaxies: high-redshift quasars: absorption lines
Keyword (fr)
Abondance Borne supérieure Densité colonne Densité élevée Déplacement vers le rouge Galaxies compagnons Métallicité Quasar Raie absorption Structure galaxies
Keyword (en)
Abundance Upper bound Column density High density Red shift Satellite galaxies Metallicity Quasars Absorption line Galaxy structure
Keyword (es)
Cota superior Densidad columna Densidad elevada Galaxias satélite Metalicidad Raya absorción Estructura galaxias
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18867885

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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