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Gamma-ray emission from pulsar/massive-star binaries

Published online by Cambridge University Press:  21 October 2010

Gustavo E. Romero
Gustavo E. Romero*
Affiliation:
Instituto Argentino de Radioastronomía (IAR, CCT La Plata, CONICET), C.C.5, (1894) Villa Elisa, Buenos Aires, Argentina email: romero@iar-conicet.gov.ar Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque s/n, 1900 La Plata, Argentina email: romero@fcaglp.unlp.edu.ar
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Abstract

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I present a review of the main phenomenological properties at high energies related to massive gamma-ray binaries and I discuss some aspects of pulsar models for these objects.

Keywords

Radiation mechanisms: non-thermalstars: neutronstars: early-typestars: windsoutflowsgamma rays: observationsgamma rays: theory
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 126 - 130
Copyright
Copyright © International Astronomical Union 2010

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