Ultraviolet dust attenuation in star-forming galaxies - II. Calibrating the A(UV) versus LTIR/LUV relation

Monthly Notices of the Royal Astronomical Society

Volumn 386, Issue 2, 2008, Pages 1157-1168

  Cortese, L ^a   Boselli, A ^b   Franzetti, P ^c   Decarli, R ^d,e   Gavazzi, G ^d   Boissier, S ^b   Buat, V ^b  

^a CARDIFF UNIVERSITY   (United Kingdom)

^b AIX MARSEILLE UNIVERSITÉ   (France)

^c INAF IASF MILANO   (Italy)

^d UNIVERSITY OF MILANO BICOCCA   (Italy)

^e UNIVERSITY OF INSUBRIA   (Italy)

Author keywords

Galaxies: evolution; Galaxies: fundamental parameters; Galaxies: general; Ultraviolet: galaxies

Indexed keywords

GALAXIES; POPULATION DISTRIBUTION; STARS;

GALAXIES GENERAL; GALAXIES: FUNDAMENTAL PARAMETERS; GALAXY EVOLUTION; PROPERTY; RATIO METHOD; SPECTRAL ENERGY DISTRIBUTION; STAR FORMATION RATES; STAR FORMING GALAXY; STELLAR POPULATIONS; ULTRAVIOLET:GALAXIES;

DUST;

EID: 42549164134     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13118.x     Document Type: Article

References (71)