Other
Scientific paper
Jul 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..593g&link_type=abstract
Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU
Other
Scientific paper
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?
Gagne Marc
Pacheco Eduardo Janot
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