Interaction-powered supernovae: Rise-time versus peak-luminosity correlation and the shock-breakout velocity

Astrophysical Journal

Volumn 788, Issue 2, 2014, Pages

  Ofek, Eran O ^a   Arcavi, Iair ^a   Tal, David ^a   Sullivan, Mark ^b   Gal Yam, Avishay ^a   Kulkarni, Shrinivas R ^c   Nugent, Peter E ^d,e   Ben Ami, Sagi ^a   Bersier, David ^f   Cao, Yi ^c   Cenko, S Bradley ^g   De Cia, Annalisa ^a   Filippenko, Alexei V ^e   Fransson, Claes ^h   Kasliwal, Mansi M ⁱ   Laher, Russ ^j   Surace, Jason ^j   Quimby, Robert ^k   Yaron, Ofer ^a  

^a WEIZMANN INSTITUTE OF SCIENCE   (Israel)

^b UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^g NASA GODDARD SPACE FLIGHT CENTER   (United States)

^h STOCKHOLM UNIVERSITY   (Sweden)

ⁱ CARNEGIE OBSERVATORIES   (United States)

^j CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^k UNIVERSITY OF TOKYO   (Japan)

more..

Author keywords

stars: mass loss; stars: massive; supernovae: general

Indexed keywords

EID: 84902204360     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/788/2/154     Document Type: Article

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