The unique type Ib supernova 2005bf: A WN star explosion model for peculiar light curves and spectra

Astrophysical Journal

Volumn 633, Issue 2 II, 2005, Pages

  Tominaga, N ^a   Tanaka, M ^a   Nomoto, K ^a,b   Mazzali, P A ^a,b,c,d   Deng, J ^e   Maeda, K ^a   Umeda, H ^a   Modjaz, M ^f   Hicken, M ^f   Challis, P ^f   Kirshner, R P ^f   Wood Vasey, W M ^f   Blake, C H ^f   Bloom, J S ^g   Skrutskie, M F ^h   Szentgyorgyi, A ^f   Falco, E E ^f   Inada, N ^a   Minezaki, T ^a   Yoshii, Y ^a   Kawabata, K ⁱ   Iye, M ^j   Anupama, G C ^k   Sahu, D K ^k   Prabhu, T P ^k   more..

^a UNIVERSITY OF TOKYO   (Japan)

^b UNIVERSITY OF TOKYO   (Japan)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^d INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^e CHINESE ACADEMY OF SCIENCES   (China)

^f HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^g UNIVERSITY OF CALIFORNIA   (United States)

^h UNIVERSITY OF VIRGINIA   (United States)

ⁱ HIROSHIMA UNIVERSITY   (Japan)

^j NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^k INDIAN INSTITUTE OF ASTROPHYSICS   (India)

more..

Author keywords

Stars: Wolf Rayet; Supernovae: general; Supernovae: individual (Cassiopeia A, SN 2005bf)

Indexed keywords

EID: 28044440708     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/498570     Document Type: Article

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