Title of article :
Do the γCas X-rays come from the Be Star?
Author/Authors :
Myron A. Smith، نويسنده , , R. Lopes de Oliveira، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2010
Abstract :
We discuss the origin of the hard X-rays in γ Cas and its analogs. Of great importance are their temporal correlations with optical/UV signatures, suggesting an origin near the Be star.
Keywords :
stars: magnetic fields , Stars: emission-line , stars: winds , Be , outflows , X-rays: stars
Journal title :
Proceedings of the International Astronomical Union
Journal title :
Proceedings of the International Astronomical Union
