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    X-ray observations of rapidly rotating O stars (1995)
    In:  CASI
    Details
    Publication Date: 2019-06-28
    Description: 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.
    Keywords: ASTRONOMY
    Type: NASA-CR-189423 , NAS 1.26:189423 , ARC-1272 , ARC-R95-236
    Format: application/pdf
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