X-ray observations of rapidly rotating O stars
Abstract
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.
- Publication:
-
Applied Research Corp. Annual Report
- Pub Date:
- May 1995
- Bibcode:
- 1995arcl.reptR....W
- Keywords:
-
- Astronomical Observatories;
- O Stars;
- Stellar Rotation;
- X Ray Astronomy;
- X Ray Sources;
- Data Reduction;
- Rosat Mission;
- Spectrometers;
- X Ray Analysis;
- Astronomy