Swift/XRT spectral analysis of MAXI J1807+132: possibility of a faint low mass X-ray binary
Abstract
We analyzed the Swift/XRT spectrum of MAXI J1807+132 obtained on March 27 in the Windowed Timing mode (Kennea et al., ATel # 10216) and found that the source could be a faint low mass X-ray binary, as suggested from optical spectroscopy (Munoz-Darias et al., ATel #10221).
- Publication:
-
The Astronomer's Telegram
- Pub Date:
- March 2017
- Bibcode:
- 2017ATel10222....1S
- Keywords:
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- Binary;
- Black Hole;
- Neutron Star;
- Transient