Long-Term Variability in Low-Mass X-Ray Binaries: A Study Using Data from VELA 5B
Abstract
A complete sample of low-mass X-ray binaries in uncrowded fields obtained from Vela 5B is studied here for periodic and aperiodic time variability on time scales of more than one day. The strong 176-day periodicity in X1820 - 303 is confirmed, and evidence is found for a significant 77-day period in Cyg X-2 and for variability on time scales of less than about 200 days in Cyg X-3. Limits are set on the possible amplitude of candidate periodicities in the literature for Ser X-1 and X0614 + 091. The evidence reported here suggests that while long-term cyclic variability is common among high-mass binaries, it is a rare occurrence in low-mass systems.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- August 1992
- DOI:
- 10.1086/171678
- Bibcode:
- 1992ApJ...395..582S
- Keywords:
-
- Fourier Analysis;
- Light Curve;
- Variable Stars;
- X Ray Binaries;
- Accretion Disks;
- Power Spectra;
- Stellar Mass;
- Astrophysics;
- STARS: BINARIES: CLOSE;
- STARS: VARIABLES: OTHER MISCELLANEOUS;
- X-RAYS: STARS