Compactified pulsar wind nebula model of gamma-ray loud binary LSI +61 303
| dc.creator | Neronov, A. | |
| dc.creator | Chernyakova, M. | |
| dc.date | 2007-01-05 | |
| dc.date.accessioned | 2026-07-07T07:38:43Z | |
| dc.date.available | 2026-07-07T07:38:43Z | |
| dc.description | We show that radio-to-TeV properties of the binary system LSI +61 303 can be explained by interaction of the compact object (a young pulsar) with the inhomogeneities of the wind from companion Be star. We develop a model scenario of "compactified" pulsar wind nebula formed in result of such interaction. To test the model assumptions about geometry of the system we re-analyze the available X-ray observations to study in more details the variations of the hydrogen column density on long (orbital) and short (several kilosecond) time scales. | |
| dc.description | submitted to MNRAS | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0701144 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0701144 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/121192 | |
| dc.subject | Astrophysics | |
| dc.title | Compactified pulsar wind nebula model of gamma-ray loud binary LSI +61 303 | |
| dc.type | text |