Spectral analysis of X-ray pulsars with the INTEGRAL observatory
| dc.creator | Filippova, E. V. | |
| dc.creator | Tsygankov, S. S. | |
| dc.creator | Lutovinov, A. A. | |
| dc.creator | Sunyaev, R. A. | |
| dc.date | 2006-10-26 | |
| dc.date.accessioned | 2026-07-07T07:27:09Z | |
| dc.date.available | 2026-07-07T07:27:09Z | |
| dc.description | We studied spectra for 34 accretion-powered X-ray and one millisecond pulsars that were within the field of view of the INTEGRAL observatory over two years (December 2002 - January 2005) of its in-orbit operation and that were detected by its instruments at a statistically significant level (>8 sigma in the energy range 18-60 keV). There are seven recently discovered objects of this class among the pulsars studied: 2RXP J130159.6-635806, IGR/AX J16320-4751, IGR J16358-4726, AX J163904-4642, IGR J16465-4507, SAX/IGR J18027-2017 and AX J1841.0-0535. We analyze the evolution of spectral parameters as a function of the intensity of the sources and compare these with the results of previous studies. | |
| dc.description | 4 pages, 1 figure, submitted proceeding of the 6th INTEGRAL Workshop "The Obscured Universe" July 2-8, 2006 Space Research Institute Moscow, Russia | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0610782 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0610782 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/117278 | |
| dc.subject | Astrophysics | |
| dc.title | Spectral analysis of X-ray pulsars with the INTEGRAL observatory | |
| dc.type | text |