The aspherical properties of the energetic type Ic SN 2002ap as inferred from its nebular spectra

Astrophysical Journal

Volumn 670, Issue 1, 2007, Pages 592-599

  Mazzali, P A ^a,b,c,d,e   Kawabata, K S ^f   Maeda, K ^a,c   Foley, R J ^g   Nomoto, K ^c,d   Deng, J ^h   Suzuki, T ^c   Iye, M ^i,j   Kashikawa, N ⁱ   Ohyama, Y ⁱ   Filippenko, A V ^g   Qiu, Y ^h   Wei, J ^h  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^c UNIVERSITY OF TOKYO   (Japan)

^d UNIVERSITY OF TOKYO   (Japan)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f HIROSHIMA UNIVERSITY   (Japan)

^g UNIVERSITY OF CALIFORNIA   (United States)

^h CHINESE ACADEMY OF SCIENCES   (China)

ⁱ NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^j GRADUATE UNIVERSITY FOR ADVANCED STUDIES   (Japan)

more..

Author keywords

Gamma rays: bursts; Nuclear reactions, nucleosynthesis, abundances; Supernovae: general; Supernovae: individual (SN 2002ap)

Indexed keywords

EID: 38349096133     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/521873     Document Type: Article

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