BeppoSAX broad-band observations of Gamma Cassiopeiae
| dc.creator | Owens, A. | |
| dc.creator | Oosterbroek, T. | |
| dc.creator | Parmar, A. N. | |
| dc.creator | Schulz, R. | |
| dc.creator | Stuwe, J. A. | |
| dc.creator | Haberl, F. | |
| dc.date | 1999-05-19 | |
| dc.date.accessioned | 2026-07-07T02:31:39Z | |
| dc.date.available | 2026-07-07T02:31:39Z | |
| dc.description | We report broad-band X-ray measurements of the Be star Gamma Cassiopeiae by the BeppoSAX X-ray astronomy satellite. The observations took place on 1998 July, 18-23. The 0.1-200 keV X-ray spectrum is reasonably well fit by an optically thin thermal plasma model of temperature 12.5 +/- 0.6 keV with significant residuals around 0.3 keV and 1 keV. The former is interpreted as the variable soft component reported by ROSAT, although there is no evidence for variability at the 5 % level. For a blackbody interpretation, the fitted temperature is 100 +320 -13 eV, in agreement with the ROSAT value of 200 +/- 10 eV. However, a MEKAL interpretation gives a significantly lower temperature of (48 +/- 11 eV). The fitted abundances are about half solar values, in agreement with previous measurements. At higher energies, the spectrum does not require non-thermal components and the observation of a line at 6.8 keV supports the ASCA interpretation of the source as an accreting white dwarf. Assuming a source distance of 188 pc, the bolometric luminosity in the 2-10 keV band is 6 10^32 erg/s. Simultaneous optical measurements by the Wendelstein Observatory near Munich, indicate that the source continues to be in a late but rather normal Be phase, with no obvious signs of a transition to the Be-shell phase. The measured magnitudes at B, V and R wavelengths of 2.18 +/- 0.06, 2.23 +/- 0.02 and 2.36 + /- 0.03, respectively, confirm this. | |
| dc.description | 5 pages. Accepted for publication in A&A | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9905245 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9905245 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14232 | |
| dc.subject | Astrophysics | |
| dc.title | BeppoSAX broad-band observations of Gamma Cassiopeiae | |
| dc.type | text |