RXTE spectra of the Galactic microquasar GRO J1655-40 during the 2005 outburst
| dc.creator | Saito, Koji | |
| dc.creator | Homan, Jeroen | |
| dc.creator | Yamaoka, Kazutaka | |
| dc.creator | Fukuyama, Mizuki | |
| dc.creator | Miyakawa, Takehiro G. | |
| dc.creator | Yoshida, Atsumasa | |
| dc.date | 2007-02-01 | |
| dc.date.accessioned | 2026-07-07T07:44:10Z | |
| dc.date.available | 2026-07-07T07:44:10Z | |
| dc.description | We report on the results of a detailed spectral analysis of 389 RXTE observations of the Galactic microquasar GRO J1655-40, performed during its 2005 outburst. The maximum luminosity reached during this outburst was 1.4 times higher than in the previous (1996-1997) outburst. However, the spectral behavior during the two outbursts was very similar. In particular, Ldisk was proportional to Tin^4 up to the same critical luminosity and in both outbursts there were periods during which the energy spectra were very soft, but could not be fit with standard disk models. | |
| dc.description | 6 pages, 5 figures, Accepted for publication in the proceedings of "Sixth Microquasar Workshop: Microquasars and Beyond", held in 18-22 September 2006 in Como, Italy, eds T. Belloni et al | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0702022 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0702022 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/123096 | |
| dc.subject | Astrophysics | |
| dc.title | RXTE spectra of the Galactic microquasar GRO J1655-40 during the 2005 outburst | |
| dc.type | text |