Precursors prior to type IIn supernova explosions are common: Precursor rates, properties, and correlations

Astrophysical Journal

Volumn 789, Issue 2, 2014, Pages

  Ofek, Eran O ^a   Sullivan, Mark ^b   Shaviv, Nir J ^c   Steinbok, Aviram ^a   Arcavi, Iair ^a   Gal Yam, Avishay ^a   Tal, David ^a   Kulkarni, Shrinivas R ^d   Nugent, Peter E ^e,f   Ben Ami, Sagi ^a   Kasliwal, Mansi M ^g   Cenko, S Bradley ^h   Laher, Russ ⁱ   Surace, Jason ⁱ   Bloom, Joshua S ^f   Filippenko, Alexei V ^f   Silverman, Jeffrey M ^j   Yaron, Ofer ^a  

^a WEIZMANN INSTITUTE OF SCIENCE   (Israel)

^b UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^c HEBREW UNIVERSITY OF JERUSALEM   (Israel)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g CARNEGIE OBSERVATORIES   (United States)

^h NASA GODDARD SPACE FLIGHT CENTER   (United States)

ⁱ CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^j The University of Texas at Austin   (United States)

more..

Author keywords

stars: mass loss; supernovae: general; supernovae: individual (SN 2010mc, PTF 10bjb, SN 2011ht, PTF 10weh, PTF 12cxj, SN 2009ip)

Indexed keywords

EID: 84903289361     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/789/2/104     Document Type: Article

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