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A 0535+26: an X-ray∕Optical Tour
- Source :
- AIP Conference Proceedings.
- Publication Year :
- 2011
- Publisher :
- AIP, 2011.
-
Abstract
- We compiled X-ray and Optical observations of the accreting X-ray binary system A 0535+262 since its discovery in 1975, that will allow us to shed light on the unpredictable behavior of this binary system. We present the data in terms of the Be-disk interaction with the neutron star companion. In addition, we show recent results from the continuous monitoring of this source by the Gamma-ray Burst Monitor(GBM), on board the Fermi observatory, since its launch in 2008 June 11.<br />Comment: 4 pages, 5 figures, Conference proceeding of "Astrophysics of Neutron Stars 2010 - a conference in honor of M. Ali Alpar", 2-6 August 2010, Cesme, Izmir, Turkey
- Subjects :
- High Energy Astrophysical Phenomena (astro-ph.HE)
Physics
Astrophysics::High Energy Astrophysical Phenomena
X-ray binary
FOS: Physical sciences
Binary number
Astrophysics
Accretion (astrophysics)
Neutron star
Pulsar
Observatory
Binary system
Astrophysics - High Energy Astrophysical Phenomena
Fermi Gamma-ray Space Telescope
Subjects
Details
- ISSN :
- 0094243X
- Database :
- OpenAIRE
- Journal :
- AIP Conference Proceedings
- Accession number :
- edsair.doi.dedup.....85780de9007145c27cd5d5a4edb28661
- Full Text :
- https://doi.org/10.1063/1.3629496