Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1085..215c&link_type=abstract
HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP Conferenc
Astronomy and Astrophysics
Astronomy
Pulsars, Gamma-Ray, Neutron Stars
Scientific paper
PSR B1259-63 is a 48 ms radio pulsar in a highly eccentric 3.4 year orbit with a Be star. Unpulsed γ-ray, X-ray and radio emission is observed from the binary system and the collision of the pulsar wind with the wind of Be star plays a crucial role in the generation of the observed emission. 2007 periastron passage was observed in unprecedented details with Suzaku, Swift, XMM-Newton and Chandra. We present here the results of this campaign, compare them with the previ observations and discuss the physical implications.
Chernyakova Maria
Kerschhaggl Matthias
Neronov Andrii
Takahashi Tadayuki
Uchiyama Yasunobu
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