Imaging the molecular gas in a submillimeter galaxy at z = 4.05: Cold mode accretion or a major merger?

Astrophysical Journal

Volumn 714, Issue 2, 2010, Pages 1407-1417

  Carilli, C L ^a   Daddi, E ^b   Riechers, D ^c   Walter, F ^d   Weiss, A ^e   Dannerbauer, H ^b   Morrison, G E ^f,g   Wagg, J ^h   Davé, Romeel ⁱ   Elbaz, D ^b   Stern, D ^j   Dickinson, M ^k   Krips, M ^l   Aravena, M ^a  

^a NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^e MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^f UNIVERSITY OF HAWAII   (United States)

^g CANADA FRANCE HAWAII TELESCOPE   (United States)

^h ESO ALMA   (Chile)

ⁱ UNIVERSITY OF ARIZONA   (United States)

^j CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^k NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^l IRAM   (France)

more..

Author keywords

Galaxies: evolution; Galaxies: formation; Galaxies: high redshift; Galaxies: ISM; Galaxies: star formation

Indexed keywords

EID: 77951690563     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/714/2/1407     Document Type: Article

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