COS-B identification of the new γ pulsar PSR 1055-52
Abstract
Using COS-B data we analyzed the timing parameters of PSR 1055-52, the newly discovered γ-ray pulsar by CGRO. We found a significant and similar pulsed structure, thus confirming the CGRO discovery. A comparison of this pulsar with 5 previously known ones is made.
- Publication:
-
Chinese Astronomy and Astrophysics
- Pub Date:
- July 1994
- DOI:
- 10.1016/0275-1062(94)90037-X
- Bibcode:
- 1994ChA&A..18..272S
- Keywords:
-
- PSR 1055;
- 52;
- γ-ray pulsar;
- timing analysis