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
Pages
2
From page
428
To page
429
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
Serial Year
2010
Journal title
Proceedings of the International Astronomical Union
Record number
667910
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