Exclusion of a Direct Progenitor Detection for the Type Ic SN 2017ein Based on Late-time Observations
To date, SN 2017ein is the only Type Ic supernova with a directly identified progenitor candidate. This candidate points to a very massive (>45 M _⊙ ) Wolf–Rayet (WR) progenitor, but its disappearance after the explosion of SN 2017ein remains unconfirmed. In this work, we revisit SN 2017ein in la...
Saved in:
Main Authors: | Yi-Han Zhao, Ning-Chen Sun, Junjie Wu, Zexi Niu, Xinyi Hong, Yinhan Huang, Justyn R. Maund, Qiang Xi, Danfeng Xiang, Jifeng Liu |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal Letters |
Subjects: | |
Online Access: | https://doi.org/10.3847/2041-8213/adad5d |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Late-time Optical and X-Ray Emission Evolution of the Oxygen-rich SN 1996cr
by: Daniel Patnaude, et al.
Published: (2025-01-01) -
Observing Supernova Neutrino Light Curves with Super-Kamiokande. V. Distance Estimation with Neutrinos
by: Yudai Suwa, et al.
Published: (2025-01-01) -
The Unique Helium Nova V445 Puppis Ejected ≫0.001 M⊙ in the Year 2000 and Will Not Become a Type Ia Supernova
by: Bradley E. Schaefer
Published: (2025-01-01) -
Investigating the Electron-capture Supernova Candidate AT 2019abn with JWST Spectroscopy
by: Sam Rose, et al.
Published: (2025-01-01) -
Nonthermal Signatures of Radiative Supernova Remnants. II. The Impact of Cosmic Rays and Magnetic Fields
by: Rebecca Diesing, et al.
Published: (2025-01-01)