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T. Sato
T. Sato
Chuo University
Type (model theory)
star
Flare
loop length
image
2
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1
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0
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The RS CVn–type Star GT Mus Shows Most Energetic X-Ray Flares Throughout the 2010s
2021
The Astrophysical Journal
R. Sasaki
Yohko Tsuboi
Wataru Iwakiri
Satoshi Nakahira
Yoshitomo Maeda
Keith C. Gendreau
Michael F. Corcoran
Kenji Hamaguchi
Zaven Arzoumanian
Craig B. Markwardt
Teruaki Enoto
T. Sato
Hiroki Kawai
Tatehiro Mihara
Megumi Shidatsu
Hitoshi Negoro
Motoko Serino
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Citations (1)
The RS CVn type star GT Mus shows most energetic X-ray flares throughout the 2010s.
2021
arXiv: High Energy Astrophysical Phenomena
R. Sasaki
Yohko Tsuboi
Wataru Iwakiri
Satoshi Nakahira
Yoshitomo Maeda
Keith C. Gendreau
Michael F. Corcoran
Kenji Hamaguchi
Zaven Arzoumanian
Craig B. Markwardt
Teruaki Enoto
T. Sato
Hiroki Kawai
Tatehiro Mihara
Megumi Shidatsu
Hitoshi Negoro
Motoko Serino
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