Hα-derived star formation rates for three z ≃ 0.75 EDisCS galaxy clusters

Astrophysical Journal

Volumn 630, Issue 1 I, 2005, Pages 206-227

  Finn, Rose A ^a,b,c   Zaritsky, Dennis ^d   McCarthy Jr , Donald W ^d   Poggianti, Bianca ^e   Rudnick, Gregory ^f   Halliday, Claire ^e,g,h,i   Milvang Jensen, B O ^h   Pelló, Roser ^j   Simard, Luc ^k  

^a NSF Astronomy and Astrophysics   (United States)

^b UNIVERSITY OF MASSACHUSETTS   (United States)

^c SIENA COLLEGE   (United States)

^d UNIVERSITY OF ARIZONA   (United States)

^e UNIVERSITY OF PADOVA   (Italy)

^f NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^g MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^h MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

ⁱ UNIVERSITY OF GÖTTINGEN   (Germany)

^j IRAP   (France)

^k NATIONAL RESEARCH COUNCIL CANADA   (Canada)

more..

Author keywords

Galaxies: clusters: general; Galaxies: evolution; Galaxies: high redshift; Stars: formation

Indexed keywords

EID: 26844439258     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/431642     Document Type: Article

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