A comparison between star formation rate diagnostics and rate of core collapse supernovae within 11 Mpc

Astronomy and Astrophysics

Volumn 537, Issue , 2012, Pages

  Botticella, M T ^a,b   Smartt, S J ^b   Kennicutt, R C ^c   Cappellaro, E ^a   Sereno, M ^d,e   Lee, J C ^f  

^a INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^b QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^d POLITECNICO DI TORINO   (Italy)

^e SEZIONE DI TORINO   (Italy)

^f Carnegie Observatories   (United States)

Author keywords

galaxies: star formation; stars: massive; supernovae: general

Indexed keywords

CORE COLLAPSE; CORE COLLAPSE SUPERNOVAE; DATA SETS; DIRECT DETECTION; FAR ULTRAVIOLET; GALAXIES: STAR FORMATION; LOWER LIMITS; MINIMUM MASS; MULTIWAVELENGTH; STAR FORMATION RATES; STARS: MASSIVE; STATISTICAL COMPARISONS; STELLAR MASS; SUPERNOVAE: GENERAL; WHITE DWARFS;

ESTIMATION; GALAXIES; LUMINANCE; SURVEYS;

STARS;

EID: 84862687657     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117343     Document Type: Article

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