The Be/X-ray Binary LSI+61303 in terms of Ejector-Propeller Model
| dc.creator | Zamanov, R. | |
| dc.creator | Marti, J. | |
| dc.creator | Marziani, P. | |
| dc.date | 2001-10-04 | |
| dc.date.accessioned | 2026-07-07T02:00:38Z | |
| dc.date.available | 2026-07-07T02:00:38Z | |
| dc.description | We tested the ejector-propeller model of the Be/X-ray binary LSI+61303 (V 615 Cas, GT 0236+620) by using the parameters predicted by the model in the calculations of the X-ray and radio variability. The results are: (1) in terms of the Ejector-Propeller model, the X-ray maximum is due to the periastron passage; (2) the radio outburst can be really a result of the transition from the propeller to ejector regimes; (3) the radio outburst will delay with respect to the X-ray maximum every orbital period. The proposed scenario seems to be in good agreement with the observations. | |
| dc.description | 9 pages, 4 figures, 2nd CNOC, "Astrophysics of Compact Objects" Sept. 19-21, 2001, Bologna, Italy | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0110114 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0110114 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3475 | |
| dc.subject | Astrophysics | |
| dc.title | The Be/X-ray Binary LSI+61303 in terms of Ejector-Propeller Model | |
| dc.type | text |