Swift/BAT X-ray monitoring indicates a new outburst of the black hole transient H 1743-322
Abstract
H 1743-322 is a black hole X-ray binary with frequent outbursts. Recent Swift/BAT monitoring observations (Krimm et al. 2013) show that this source has turned into a new outburst after been in quiescence for about nine months since the most recent outburst in 2016.
- Publication:
-
The Astronomer's Telegram
- Pub Date:
- July 2017
- Bibcode:
- 2017ATel10599....1Z
- Keywords:
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- Binary;
- Black Hole;
- Transient