New Perspectives on B Star X-ray Emission: The High-Resolution X-Ray Spectra of Spica and β Cen

Details New Perspectives on B Star X-ray Emission: The High-Resolution X-Ray Spectra of Spica and β Cen New Perspectives on B Star X-ray Emission: The High-Resolution X-Ray Spectra of Spica and β Cen

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361...77m&link_type=abstract

Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere

Physics

1

Scientific paper

The advent of high-resolution X-ray spectroscopy has provided a number of new ways to probe the X-ray emission of B stars, resulting in a large amount of new information which has been difficult to develop into a simple framework. This paper concentrates on the X-ray spectra of Spica and β Cen, two β Cep variables which are in other respects typical B stars. Three main topics are discussed: their X-ray line profiles, the f/i ratios from He-like ions, and their X-ray lightcurves.

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