Chandra HETGS Observations of B Supergiants

Details Chandra HETGS Observations of B Supergiants Chandra HETGS Observations of B Supergiants

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..774..353w&link_type=abstract

X-RAY DIAGNOSTICS OF ASTROPHYSICAL PLASMAS: Theory, Experiment, and Observation. AIP Conference Proceedings, Volume 774, pp. 35

Astronomy and Astrophysics

Astrophysics

5

Supergiant Stars, X-Ray Sources (Astronomical), Supergiant Stars, X-Ray, Mass Loss And Stellar Winds, Main-Sequence: Early-Type Stars

Scientific paper

Preliminary results from the first HETGS observation of an early B supergiant, ɛ Orionis (B0 Ia), are presented. The observed emission line spectrum and X-ray emission line characteristics are compared to those of previous O-star studies. In addition, the significance of the observed stellar wind distribution of X-ray temperatures, as determined from several OB stars, is discussed.

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