Relation between supersoft X-ray sources and VY Scl stars
| dc.creator | Greiner, Jochen | |
| dc.creator | DiStefano, Rosanne | |
| dc.date | 1998-10-01 | |
| dc.date.accessioned | 2026-07-07T02:28:10Z | |
| dc.date.available | 2026-07-07T02:28:10Z | |
| dc.description | In a recent ROSAT observation, taken during its optical low state, we found that the VY Scl star V751 Cyg was a highly luminous source of soft X-rays. The ROSAT HRI count rate of V751 Cyg was a factor of 10-20 higher than upper limits obtained with ROSAT during previous observations, during which V751 Cyg happened to be in the optical high state. Analysis of the X-ray spectrum suggests a very low temperature (kT~15 eV) and a bolometric luminosity of 5*10^36 (D/500 pc)^2 erg/s. These values are characteristic of supersoft X-ray sources. Based on the supersoft nature of V751 Cyg and the similarity of the variability pattern of VY Scl stars and the supersoft transient source RX J0513.9-6951 we hypothezise a relation between VY Scl stars and supersoft X-ray sources. It is conceivable that VY Scl stars are all supersoft binaries (SSB), that they form an extension of the previously known class of SSBs towards lower white dwarf masses and lower temperatures. | |
| dc.description | 4 pages (modified aa style using xray_symp.cls) incl. 3 figures, Proc. of Highlights in X-ray Astronomy'', eds. B. Aschenbach et al., Garching, June 1998, to appear as MPE Report; also available from http://www.obs.aip.de/~jcg/publis.html | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9810019 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9810019 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13008 | |
| dc.subject | Astrophysics | |
| dc.title | Relation between supersoft X-ray sources and VY Scl stars | |
| dc.type | text |