X-ray observations of rapidly rotating O stars

Details X-ray observations of rapidly rotating O stars X-ray observations of rapidly rotating O stars

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995arcl.reptr....w&link_type=abstract

Final Report Applied Research Corp., Landover, MD.

Astronomy and Astrophysics

Astronomy

Astronomical Observatories, O Stars, Stellar Rotation, X Ray Astronomy, X Ray Sources, Data Reduction, Rosat Mission, Spectrometers, X Ray Analysis

Scientific paper

HEAO-2 results suggest that high vsini O stars appear to be significantly fainter x-ray sources. We proposed to observe additional high vsini O stars to test this hypothesis. Unfortunately, the PSPC was shot down during our scheduled observation time, and the observation was not re-scheduled. The contract work was modified to carry out other related x-ray tasks.

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