The role of galaxy interaction in the SFR-M * relation: Characterizing morphological properties of herschel-selected galaxies at 0.2 < z < 1.5

Astrophysical Journal

Volumn 778, Issue 2, 2013, Pages

  Hung, Chao Ling ^a   Sanders, D B ^a   Casey, C M ^a   Lee, N ^a   Barnes, J E ^a   Capak, P ^b   Kartaltepe, J S ^c   Koss, M ^a   Larson, K L ^a   Le Floc'H, E ^d   Lockhart, K ^a   Man, A W S ^a,e   Mann, A W ^a   Riguccini, L ^f,g   Scoville, N ^h   Symeonidis, M ^i,j  

^a UNIVERSITY OF HAWAII   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^d CEA SACLAY   (France)

^e UNIVERSITY OF COPENHAGEN   (Denmark)

^f NASA AMES RESEARCH CENTER   (United States)

^g BAER Institute   (United States)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ UNIVERSITY OF SUSSEX   (United Kingdom)

^j UNIVERSITY COLLEGE LONDON   (United Kingdom)

more..

Author keywords

galaxies: evolution; galaxies: structure; infrared: galaxies

Indexed keywords

EID: 84887908113     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/778/2/129     Document Type: Article

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