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Highly Luminous SNe Associated with GRBs

Poster on-line

Published online by Cambridge University Press:  29 August 2019

D. A. Kann*
Affiliation:
Instituto Astrofísica de Andalucía (CSIC), Granada, Spain email: [email protected]
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Abstract

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The broad-lined Type Ic Supernovæ (SNe) associated with Gamma-Ray Bursts (GRBs) were long considered the most luminous class as a whole among core-collapse SNe, until the discovery of Superluminous SNe (SLSNe) during the last decade. There are many differences between the two classes, but in recent years events have been discovered which form a link between them. Associated with GRBs but more luminous and hotter, and in one case clearly dissimilar spectrally from any other known GRB-SNe, these sources point the way towards common mechanisms underlying GRBs and SLSNe.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

Footnotes

Supplementary material: PDF

Kann supplementary material

Kann supplementary material

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