On the Nature of the Underlying Star associated with Sco X-l

Details On the Nature of the Underlying Star associated with Sco X-l On the Nature of the Underlying Star associated with Sco X-l

May 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970natur.226..432f&link_type=abstract

Nature, Volume 226, Issue 5244, pp. 432-434 (1970).

Physics

10

Scientific paper

IN a recent report1 we presented evidence for the existence of short-term periodic variations in the optical ``flickering'' of Sco X-l following a large (optical) flare on the night of April 3, 1967. We now have reason to believe that the pronounced feature that was found at approximately 0.006 Hz in the power spectrum of the immediately postflare data sample (610-1,109 of the photometric observations by Sandage et al.2) can be explained in terms of the acoustic oscillations of a hot, bounded plasma atmosphere in the strong gravitational field of a dense underlying star.

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