The radial distribution of core-collapse supernovae in spiral host galaxies

Astronomy and Astrophysics

Volumn 508, Issue 3, 2009, Pages 1259-1268

  Hakobyan, A A ^a   Mamon, G A ^b,c   Petrosian, A R ^a   Kunth, D ^b   Turatto, M ^d  

^a BYURAKAN ASTROPHYSICAL OBSERVATORY   (Armenia)

^b INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^c UNIVERSITY OF OXFORD   (United Kingdom)

^d INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

Author keywords

Galaxies: spiral; Galaxies: stellar content; Supernovae: general

Indexed keywords

EXPONENTIAL DISTRIBUTIONS; EXPONENTIAL LAW; GALAXIES: SPIRALS; H II REGIONS; HOST GALAXIES; INITIAL MASS; INNER REGION; IONIZED GAS; LENGTH NORMALIZATION; MASSIVE STARS; METALLICITIES; RADIAL DISTANCE; RADIAL DISTRIBUTIONS; SCALE LENGTH; STELLAR DISKS; SUPERNOVAE: GENERAL; TYPE II; GALAXIES: STELLAR CONTENT;

DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); GASES; IONIZATION OF GASES; STARS; ASTROPHYSICS;

GALAXIES;

EID: 72849119039     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912795     Document Type: Article

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