Star formation history of galaxies from z = 0 to z = 0.7: A backward approach to the evolution of star-forming galaxies

Astronomy and Astrophysics

Volumn 483, Issue 1, 2008, Pages 107-119

  Buat, V ^a   Boissier, S ^a   Burgarella, D ^a   Takeuchi, T ^b   Le Floc'H, E ^c   Marcillac, D ^d   Huang, J ^e   Nagashima, M ^f   Enoki, M ^g  

^a AIX MARSEILLE UNIVERSITÉ   (France)

^b NAGOYA UNIVERSITY   (Japan)

^c UNIVERSITY OF HAWAII   (United States)

^d UNIVERSITY OF ARIZONA   (United States)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f NAGASAKI UNIVERSITY   (Japan)

^g TOKYO KEIZAI UNIVERSITY   (Japan)

Author keywords

Galaxies: evolution; Galaxies: stellar content; Infrared: galaxies; Ultraviolet: galaxies

Indexed keywords

INFRARED RADIATION; MATHEMATICAL MODELS; STARS; ULTRAVIOLET RADIATION;

SPECIFIC STAR FORMATION RATE (SSFR); SPIRAL GALAXIES; STELLAR CONTENT;

GALAXIES;

EID: 43049109556     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078263     Document Type: Article

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