Non-pulsing emission from X-ray pulsars
| dc.creator | Lutovinov, A. | |
| dc.creator | Grebenev, S. | |
| dc.creator | Sunyaev, R. | |
| dc.date | 2001-06-13 | |
| dc.date.accessioned | 2026-07-07T01:58:54Z | |
| dc.date.available | 2026-07-07T01:58:54Z | |
| dc.description | Results of GRANAT/ART-P observations of three X-ray pulsars in non-pulsing states are presented: 1) a statistically significant non-pulsing flux with a simple power-law spectrum was detected during the ``off''- state of Her X-1; 2) a significant (13 $σ$) non-pulsing flux with a strong iron emission line at energies ~ 6.7-6.9 keV was detected during the eclipse ingress of Cen X-3; 3) a weak non-pulsing flux was detected during the X-ray eclipse of Vela X-1, which probably resulted from scattering of the pulsar emission in the stellar wind of an optical star. | |
| dc.description | 2 pages, to appear in the proceedings of the "New Century of X-ray Astronomy" symposium, ASP press | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0106237 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0106237 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2901 | |
| dc.subject | Astrophysics | |
| dc.title | Non-pulsing emission from X-ray pulsars | |
| dc.type | text |