Quasi-periodic oscillations in GX 17+2.
Abstract
X-ray observations of GX 17 + 2 were made in March and April, 1988 with the Large Area Counter of the Ginga satellite. The source was observed in the flaring, normal, and horizontal branches. Quasi-periodic oscillations (QPOs) were oberved in all three of these branches. The relationship between QPO behavior and the X-ray spectral properties of GX 17 + 2 is examined. Continuous variation of QPO behavior is observed as GX 17 + 2 moves from the normal to flaring branch, indicating that the normal-branch QPO and the flaring-branch QPO are probably one physical phenomenon. This QPO behavior is similar to that observed in Sco X-1. Also, it is found that GX 17 + 2 is an example of the Z-type sources defined by Hasinger et al. (1989).
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- March 1990
- DOI:
- 10.1093/mnras/243.1.114
- Bibcode:
- 1990MNRAS.243..114P
- Keywords:
-
- Astronomical Spectroscopy;
- Galactic Bulge;
- Oscillations;
- X Ray Sources;
- Astronomical Observatories;
- Color-Color Diagram;
- Power Spectra;
- Radio Emission;
- Astrophysics