A BeppoSAX LECS observation of the super-soft X-ray source CAL 83
Abstract
We report on a BeppoSAX Low-Energy Concentrator Spectrometer (LECS) observation of the super-soft source (SSS) CAL 83. The X-ray emission in SSS is believed to arise from nuclear burning of accreted material on the surface of a white dwarf (WD). The LECS spectrum of CAL 83 can be well fit by both absorbed blackbody and WD atmosphere models. If the absorption is constrained to be equal to the value derived from Hubble Space Telescope measurements, then the best-fit blackbody temperature is 46.4 +/- 1.4 eV while a Non Local Thermal Equilibrium (NLTE) WD atmosphere model gives a lower temperature of 32.6 +/- 0.7 eV. In contrast to CAL87, there are no strong absorption edges visible in the X-ray spectrum with a 68% confidence upper limit of 2.3 to the optical depth of a C {s(-1) c vi} edge at 0.49 keV predicted by WD atmosphere models. The luminosity and radius derived from the NLTE fit are consistent with the values predicted for stable nuclear burning on the surface of a s^{-1}im0.9-1.0Msun WD.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- April 1998
- DOI:
- 10.48550/arXiv.astro-ph/9712040
- arXiv:
- arXiv:astro-ph/9712040
- Bibcode:
- 1998A&A...332..199P
- Keywords:
-
- ACCRETION;
- ACCRETION DISKS;
- BINARIES: CLOSE;
- STARS: INDIVIDUAL: CAL 83;
- WHITE DWARFS -X-RAYS: STARS;
- Astrophysics
- E-Print:
- 5 pages. Accepted for publication in A&