Hard X-rays from Be star LSI +61degr 303

Details Hard X-rays from Be star LSI +61degr 303 Hard X-rays from Be star LSI +61degr 303

Feb 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...366..865a&link_type=abstract

Astronomy and Astrophysics, v.366, p.865-867 (2001)

Astronomy and Astrophysics

Astrophysics

3

X-Ray Source, Be Star, Lsi +61Degr 303

Scientific paper

We show that the hard X-ray emission from the X-ray source LSI +61degr
303 can be due to inverse Compton scattering of optical photons from the
Be star by the relativistic electrons responsible for the observed radio
emission.

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