A search for cyclotron resonance features with INTEGRAL
| dc.creator | Okada, Y. | |
| dc.creator | Niko, H. | |
| dc.creator | Kokubun, M. | |
| dc.creator | Makishima, K. | |
| dc.creator | Nakajima, M. | |
| dc.creator | Mihara, T. | |
| dc.creator | Terada, Y. | |
| dc.creator | Nagase, F. | |
| dc.creator | Tanaka, Y. | |
| dc.date | 2004-06-21 | |
| dc.date.accessioned | 2026-07-07T02:13:36Z | |
| dc.date.available | 2026-07-07T02:13:36Z | |
| dc.description | We present an INTEGRAL observation of the Cen-Crux region in order to search the electron cyclotron resonance scattering features from the X-ray binary pulsars. During the AO1 200ks observation, we clearly detected 4 bright X-ray binaries, 1 Seyfert Galaxy, and 4 new sources in the field of view. Especially from GX301-2, the cyclotron resonance feature is detected at about 37 keV, and width of 3--4 keV. In addition, the depth of the resonance feature strongly depends on the X-ray luminosity. This is the first detection of luminosity dependence of the resonance depth. The cyclotron resonance feature is marginally detected from 1E1145.1-6141. Cen X-3 was very dim during the observation and poor statistics disable us to detect the resonance features.These are first INTEGRAL results of searching for the cyclotron resonance feature. | |
| dc.description | 4pages, 8figures, To be published in the Proceedings of the 5th INTEGRAL Workshop: "The INTEGRAL Universe", February 16-20, 2004, Munich | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0406449 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0406449 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7867 | |
| dc.subject | Astrophysics | |
| dc.title | A search for cyclotron resonance features with INTEGRAL | |
| dc.type | text |