4U 1145-61
Abstract
N. E. White, Mullard Space Sciences Laboratory, reports that Ariel 5 observations centered on 4U 1145-61 during Sept. 20-Oct. 4 have revealed x-ray pulsations with a period of 4.954 +/- 0.004 min. Variations in this period indicate orbital motion with a period of 14-18 days. The optical candidate HD 102567 has been proposed.
- Publication:
-
International Astronomical Union Circular
- Pub Date:
- October 1977
- Bibcode:
- 1977IAUC.3118....1W