Non-radial Optical Pulsations in SXP 175 (RX J0101.8-7223)
Abstract
SXP 175 was discovered as an X-ray pulsar by Townsend et al. (ATel #3311). The source's position was coincident with RX J0101.8-7223, which had been identified with the emission-line star MA[93] 1288.
- Publication:
-
The Astronomer's Telegram
- Pub Date:
- September 2019
- Bibcode:
- 2019ATel13128....1S
- Keywords:
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- Binary;
- Neutron Star;
- Pulsar