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A SUPER-DAMPED Lyα QUASI-STELLAR OBJECT ABSORBER AT z = 2.2

Author
KULKARNI, Varsha P1 ; MEIRING, Joseph2 ; SOM, Debopam1 ; PEROUX, Celine3 ; YORK, Donald G4 ; KHARE, Pushpa5 ; LAUROESCH, James T6
[1] Department of Physics and Astronomy, University of South Carolina, Columbia, SC 29208, United States
[2] Department of Astronomy, University of Massachusetts, Amherst, MA 01003, United States
[3] Laboratoire d'Astrophysique de Marseille, OAMP, Universite Aix-Marseille, 13388 Marseille, France
[4] Department of Astronomy & Astrophysics, University of Chicago, Chicago, IL 60637, United States
[5] Inter-University Center for Astronomy & Astrophysics, Pune 411007, India
[6] Department of Physics & Astronomy, University of Louisville, Louisville. KY 40292, United States
Source

The Astrophysical journal. 2012, Vol 749, Num 2 ; 176.1-176.14 ; 1 ; ref : 3/4 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
dust, extinction quasars: absorption lines
Keyword (fr)
Abondance élément Atténuation Courbe extinction Densité électron Etude ciel Formation stellaire Grand Nuage Magellan Métallicité Petit Nuage Magellan Quasar Raie Lyman alpha Raie absorption Source gamma cosmique Spectrométrie Sursaut Rγ Taux formation Voie lactée
Keyword (en)
Element abundance Attenuation Extinction curve Electron density Sky surveys Star formation Large Magellanic Cloud Metallicity Small Magellanic Cloud Quasars Lyman alpha line Absorption line Cosmic gamma sources Spectroscopy Gamma ray burst Formation rate Milky Way
Keyword (es)
Curva extinción Metalicidad Raya Lyman alfa Raya absorción Arrebato Rγ Grado formación
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
25796448

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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