Handbook of Supernovae

By A. W. Alsabti, P. Murdin. 2017

299 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/9fa58cb83d47ee864f845d71aaae63184b647484

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In Astronomy and Astrophysics

1. A. Gal-yam

Citations in the corpus

• The Most Luminous Supernovae (2018, background): “CSM interaction is likely responsible for powering hydrogen rich type IIn SNe, heliumrich SNe Ibn, rare luminous SN Ia explosions (Ia-CSM) and even some SNe Ic (see Gal-Yam 2017 for a recent review of these SN classes).”
• The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole? (2018, unknown): “Most corecollapse SNe are believed to exhibit an early shock-breakout and shock-cooling phase in which the stellar photosphere is nearly-instantaneously heated to X-ray temperatures by the emergence of the SN shock, producing a rapid rise in the light curve (Waxman & Katz 2017).”