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titleProbing the Pulsar Wind in the gamma-ray Binary System: PSR B1259-63/SS 2883
Author(eng)Takata, Jumpei; Taam, Ronald E.
Author Affiliation(eng)Department of Physics, University of Hong Kong; Academia Sinica Institute of Astrophysics and Astronomy-TIARA
Issue Date2010-02-26
Publisher宇宙航空研究開発機構
Japan Aerospace Exploration Agency (JAXA)
Publication title宇宙航空研究開発機構特別資料:
JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H
VolumeJAXA-SP-09-008E
Start page50
End page51
Publication date2010-02-26
Languageeng
AbstractThe spectral energy distribution from the X-ray to the very high energy regime (> 100 GeV) has been investigated for the gamma-ray binary system PSR B1259-63/SS2883 as a function of orbital phase within the framework of a simple model of a pulsar wind nebula. The emission model is based on the synchrotron radiation process for the X-ray regime and the inverse Compton scattering process boosting stellar photons from the Be star companion to the very high energy (100GeV-TeV) regime. With this model, the observed temporal behavior can, in principle, be used to probe the pulsar wind properties at the shock as a function of the orbital phase.
DescriptionMeeting Information: The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan
Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science
Keywordsacceleration of particles - radiation mechanisms: non-thermal - gamma rays: theory - Xrays: binaries - pulsars: individual (PSR B1259-63)
Document TypeConference Paper
JAXA Category特別資料
ISSN1349-113X
NCIDAA11984031
SHI-NOAA0064574019
Report NoJAXA-SP-09-008E
URIhttps://repository.exst.jaxa.jp/dspace/handle/a-is/21837


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