Literature DB >> 24132286

Astrophysics: Super-luminous supernovae on the rise.

Daniel Kasen.   

Abstract

Year:  2013        PMID: 24132286     DOI: 10.1038/502310a

Source DB:  PubMed          Journal:  Nature        ISSN: 0028-0836            Impact factor:   49.962


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  5 in total

1.  Pulsational pair instability as an explanation for the most luminous supernovae.

Authors:  S E Woosley; S Blinnikov; Alexander Heger
Journal:  Nature       Date:  2007-11-15       Impact factor: 49.962

2.  Slowly fading super-luminous supernovae that are not pair-instability explosions.

Authors:  M Nicholl; S J Smartt; A Jerkstrand; C Inserra; M McCrum; R Kotak; M Fraser; D Wright; T-W Chen; K Smith; D R Young; S A Sim; S Valenti; D A Howell; F Bresolin; R P Kudritzki; J L Tonry; M E Huber; A Rest; A Pastorello; L Tomasella; E Cappellaro; S Benetti; S Mattila; E Kankare; T Kangas; G Leloudas; J Sollerman; F Taddia; E Berger; R Chornock; G Narayan; C W Stubbs; R J Foley; R Lunnan; A Soderberg; N Sanders; D Milisavljevic; R Margutti; R P Kirshner; N Elias-Rosa; A Morales-Garoffolo; S Taubenberger; M T Botticella; S Gezari; Y Urata; S Rodney; A G Riess; D Scolnic; W M Wood-Vasey; W S Burgett; K Chambers; H A Flewelling; E A Magnier; N Kaiser; N Metcalfe; J Morgan; P A Price; W Sweeney; C Waters
Journal:  Nature       Date:  2013-10-17       Impact factor: 49.962

3.  Supernova 2007bi as a pair-instability explosion.

Authors:  A Gal-Yam; P Mazzali; E O Ofek; P E Nugent; S R Kulkarni; M M Kasliwal; R M Quimby; A V Filippenko; S B Cenko; R Chornock; R Waldman; D Kasen; M Sullivan; E C Beshore; A J Drake; R C Thomas; J S Bloom; D Poznanski; A A Miller; R J Foley; J M Silverman; I Arcavi; R S Ellis; J Deng
Journal:  Nature       Date:  2009-12-03       Impact factor: 49.962

4.  Superluminous supernovae at redshifts of 2.05 and 3.90.

Authors:  Jeff Cooke; Mark Sullivan; Avishay Gal-Yam; Elizabeth J Barton; Raymond G Carlberg; Emma V Ryan-Weber; Chuck Horst; Yuuki Omori; C Gonzalo Díaz
Journal:  Nature       Date:  2012-10-31       Impact factor: 49.962

5.  Hydrogen-poor superluminous stellar explosions.

Authors:  R M Quimby; S R Kulkarni; M M Kasliwal; A Gal-Yam; I Arcavi; M Sullivan; P Nugent; R Thomas; D A Howell; E Nakar; L Bildsten; C Theissen; N M Law; R Dekany; G Rahmer; D Hale; R Smith; E O Ofek; J Zolkower; V Velur; R Walters; J Henning; K Bui; D McKenna; D Poznanski; S B Cenko; D Levitan
Journal:  Nature       Date:  2011-06-08       Impact factor: 49.962

  5 in total

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