Pulse Frequency Changes of 1E 2259+586 and the Binary Interpretation
Abstract
Pulse frequencies from the archival ROSAT observations of lE 2259+586 are presented. A short-term spin-up episode superposed on the secular spin-down trend is observed. Combining the previously published pulse frequencies, we estimate the variance of the angular velocity over a 15 yr span of observations. The level of fluctuations in angular velocity is similar to that of established accreting binary neutron stars. These results favor accretion by a neutron star from a very low mass companion as the source of the X-ray luminosity, although accretion by a solitary neutron star from a residual disk might be possible.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- March 1996
- DOI:
- 10.1086/176985
- Bibcode:
- 1996ApJ...460..470B
- Keywords:
-
- STARS: BINARIES: CLOSE;
- STARS: PULSARS: INDIVIDUAL ALPHANUMERIC: 1E 2259+586;
- X-RAYS: STARS