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High resolution X-ray spectroscopy of bright O type stars

Monthly Notices of the Royal Astronomical Society, no. 1 (2006): 313-326

Cited by: 64|Views5
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Abstract

Archival X-ray spectra of the four prominent single, non-magnetic O stars ζ Pup, ζ Ori, ξ Per and ζ Oph, obtained in high resolution with Chandra HETGS/MEG have been studied. The resolved X-ray emission line profiles provide information about the shocked, hot gas which emits the X-radiation, and about the bulk of comparably cool stellar w...More

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