Radio Follow-up Observations of SN 2023ixf by Japanese and Korean Very Long Baseline Interferometers

Radio Follow-up Observations of SN 2023ixf by Japanese and Korean Very Long Baseline Interferometers

We report on radio follow-up observations of the nearby Type II supernova SN 2023ixf, spanning from 1.7 to 269.9 days after the explosion, conducted using three very long baseline interferometers (VLBIs), which are the Japanese VLBI Network, the VLBI Exploration of Radio Astrometry, and the Korean V...

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Bibliographic Details
Main Authors: Yuhei Iwata, Masanori Akimoto, Tomoki Matsuoka, Keiichi Maeda, Yoshinori Yonekura, Nozomu Tominaga, Takashi J. Moriya, Kenta Fujisawa, Kotaro Niinuma, Sung-Chul Yoon, Jae-Joon Lee, Taehyun Jung, Do-Young Byun
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Supernovae
Core-collapse supernovae
Type II supernovae
Massive stars
Red supergiant stars
Stellar mass loss
Online Access:https://doi.org/10.3847/1538-4357/ad9a62
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https://doi.org/10.3847/1538-4357/ad9a62

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