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Discussion – Normal and active OB stars as extreme condition test beds

Published online by Cambridge University Press:  12 July 2011

Marc Gagné  and
Eduardo Janot Pacheco
Marc Gagné
Affiliation:
West Chester University, USA
Eduardo Janot Pacheco
Affiliation:
Universidade de Sao Paulo, Brazil
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Guillaume Dubus: As far as I can tell your model is exactly the same as standard models for high-mass x-ray binaries, the on difference is that you have a mechanism for generating γ rays. My question is, we know that there are dozens of other systems that are just LS 5039, so why are they not emitting γ rays?

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 593 - 599
Copyright
Copyright © International Astronomical Union 2011