Observations of SN 2017ein Reveal Shock Breakout Emission and a Massive Progenitor Star for a Type Ic Supernova-Reference-Cited by-同舟云学术

Observations of SN 2017ein Reveal Shock Breakout Emission and a Massive Progenitor Star for a Type Ic Supernova

Published:2019-01-30 Issue:2 Volume:871 Page:176
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Xiang Danfeng,Wang Xiaofeng^ORCID,Mo Jun,Wang Lingjun^ORCID,Smartt Stephen^ORCID,Fraser Morgan^ORCID,Ehgamberdiev Shuhrat A.,Mirzaqulov Davron,Zhang Jujia^ORCID,Zhang Tianmeng^ORCID,Vinko Jozsef^ORCID,Wheeler J. Craig^ORCID,Hosseinzadeh Griffin^ORCID,Howell D. Andrew,McCully Curtis^ORCID,DerKacy James M,Baron E.^ORCID,Brown Peter^ORCID,Zhang Xianfei^ORCID,Bi Shaolan^ORCID,Song Hao,Zhang Kaicheng,Rest A.,Nomoto Ken’ichi^ORCID,Tolstov Alexey^ORCID,Blinnikov Sergei

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/871/i=2/a=176/pdf

Reference111 articles.

1. Constraints on the Progenitor of SN 2016gkg from Its Shock-cooling Light Curve

2. Type I supernovae. I - Analytic solutions for the early part of the light curve

3. The Chemical Composition of the Sun

4. LSQ14efd: observations of the cooling of a shock break-out event in a type Ic Supernova

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