Modulation of the high energy γ-ray flux from PSR B1259-63/SS2883 due to the orbital variation of the maximum energy of ... View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2007

AUTHORS

Dmitry Khangulyan , Slavomir Hnatic , Felix Aharonian

ABSTRACT

The inverse Compton (IC) scattering of ultrarelativistic electrons accelerated at the pulsar wind termination shock is generally believed to be responsible for TeV gamma-ray signal recently reported from the binary system PSR B1259-63/SS2883. In such a system the acceleration takes place in the presence of a dense radiation field provided by a companion Be2-type star. Thus it is natural to expect an orbital phase dependence of the acceleration efficiency in the system. The HESS collaboration reported the tendency of reduction of TeV γ-rays around the periastron. In this paper we study a possible explanation of this effect by the “early” (sub-TeV) cutoffs in the energy spectrum of accelerated electrons due to the enhanced rate of Compton losses close to the periastron. More... »

PAGES

261-265

Book

TITLE

The Multi-Messenger Approach to High-Energy Gamma-Ray Sources

ISBN

978-1-4020-6117-2
978-1-4020-6118-9

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-1-4020-6118-9_40

DOI

http://dx.doi.org/10.1007/978-1-4020-6118-9_40

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1031631981


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