Some Considerations on the HMXRB LSI +61 303

Details Some Considerations on the HMXRB LSI +61 303 Some Considerations on the HMXRB LSI +61 303

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..217p&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

Scientific paper

We discuss the spectral variations of the runaway Be star LSI +61 303 (V
615 Cas), the optical counterpart of the hard X-ray source source RX
J0240.4+6112.

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