Spectral states and transient behaviour of a sample of X-ray bursters observed by BeppoSax
| dc.creator | Natalucci, L. | |
| dc.creator | Bazzano, A. | |
| dc.creator | Capitanio, F. | |
| dc.creator | Cocchi, M. | |
| dc.creator | Ubertini, P. | |
| dc.creator | Zand, J. J. M. in 't | |
| dc.date | 2004-08-03 | |
| dc.date.accessioned | 2026-07-07T02:14:11Z | |
| dc.date.available | 2026-07-07T02:14:11Z | |
| dc.description | During observation campaigns of the Galactic Bulge region, BeppoSAX detected a total of 21 new X-ray bursters in about 6 years of operation. These sources are mostly transient and often feature a hard X-ray spectrum, extending up to ~ 200 keV. A hard spectrum is generally found in weak, relatively short outbursts. On the other hand two sources, SAX J1747.0-2853 and SAX J1750.8-2900, have been seen with soft X-ray transient behaviour. In both low/hard and high/soft state, a thermal component is observed at energies below \~10 keV and the spectra are compatible with the same model consisting of a blackbody or disk blackbody plus a hard or Comptonized component. Light curves are characterized by either weak, short flares or longer, high luminosity eruptions with exponential decay. | |
| dc.description | 4 pages, 6 figures, to appear in Proceedings of the 5th INTEGRAL Workshop 'The INTEGRAL Universe', Munich, 16-20 February 2004. Accepted for publication in ESA SP-552 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0408046 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0408046 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8022 | |
| dc.subject | Astrophysics | |
| dc.title | Spectral states and transient behaviour of a sample of X-ray bursters observed by BeppoSax | |
| dc.type | text |