INTEGRAL detection of bright hard X-ray emission from the RS CVn star GT Mus
Abstract
The RS CVn star GT Mus is currently undergoing X-ray activity as detected by MAXI/GSC (Atel#9251) starting on 2016-07-16 13:08:30 UT (trigger time). The 4-10 keV flux (about 150 mCrab) is among the highest ones measured with the MAXI/GSC.
- Publication:
-
The Astronomer's Telegram
- Pub Date:
- July 2016
- Bibcode:
- 2016ATel.9255....1S
- Keywords:
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- Star;
- Transient