Identifying dynamically young galaxy groups via wide-angle tail galaxies: A case study in the cosmos field at z = 0.53

Astrophysical Journal

Volumn 713, Issue 1, 2010, Pages 484-490

  Oklopcic A ^a,b   Smolcic V ^b,c,d   Giodini, S ^e   Zamorani, G ^f   Brzan, L ^g   Schinnerer, E ^h   Carilli, C L ⁱ   Finoguenov, A ^e   Lilly, S ^j   Koekemoer, A ^k   Scoville, N Z ^b  

^a UNIVERSITY OF ZAGREB   (Croatia)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^d UNIVERSITY OF BONN   (Germany)

^e MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^f INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^g LEIDEN UNIVERSITY   (Netherlands)

^h MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

ⁱ NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^j ETH ZURICH   (Switzerland)

^k STScI   (United States)

more..

Author keywords

Cosmology: observations; Galaxies: active; Galaxies: evolution; Galaxies: fundamental parameters; Radio continuum: galaxies

Indexed keywords

EID: 77950244136     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/713/1/484     Document Type: Article

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