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19962023
most citedThe Magnetorotational Instability in Core Collapse Supernova Explosions

435 citations · 12.3k across the 206 of their papers we have counts for

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Showing 2018Show all

9 papers · 1 filter

astro-ph.HE2018★ 46 cited

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

Danfeng Xiang, Xiaofeng Wang, Jun Mo +23

We present optical and ultraviolet observations of nearby type Ic supernova SN 2017ein as well as detailed analysis of its progenitor properties from both the early-time observatio…

astro-ph.SR2018★ 85 cited

Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the 2 Observations

W. Li, X. Wang, J. Vinkó +160

Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the field. The data revealed an excess emission…

astro-ph.SR2018★ 19 cited

RINGO3 polarimetry of the Type I superluminous SN 2017egm

J. R. Maund, I. Steele, H. Jermak +2

The origin of the luminosity of superluminous supernovae (SLSNe) is an unresolved mystery, and a number of very different physical scenarios (including energy injection from magnet…

astro-ph.SR2018★ 5 cited

SN 2014J in M82: New Insights On the Spectral Diversity of Type Ia Supernovae

Kaicheng Zhang, Xiaofeng Wang, JuJia Zhang +25

We present extensive spectroscopic observations for one of the closest type Ia supernovae (SNe Ia), SN 2014J discovered in M82, ranging from 10.4 days before to 473.2 days after B-…

astro-ph.HE2018★ 77 cited

X-ray Swift observations of SN 2018cow

L. E. Rivera Sandoval, T. J. Maccarone, A. Corsi +3

Supernova (SN) 2018cow (or AT2018cow) is an optical transient detected in the galaxy CGCG 137-068. It has been classified as a SN due to various characteristics in its optical spec…

astro-ph.SR2018★ 12 cited

The Betelgeuse Project II: Asteroseismology

S. Nance, J. M. Sullivan, M. Diaz +1

We explore the question of whether the interior state of massive red supergiant supernova progenitors can be effectively probed with asteroseismology. We have computed a suite of t…