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Wheaton, W. A.

Publications and source records attributed to Wheaton, W. A..

58 records · Page 4

Observations of the binary X-ray source SMC X-1 from OSO-7.

The X-ray source was observed with an X-ray telescope during the time from April 15, 1972 to May 25, 1972. These observations complement the Uhuru results reported by Schreier et al. (1972) and permit an extension of the spectrum to at least 35 keV. Combined with other observations, the data could help determine long term periodic variations, if any exist. The relative exposure and the corrected counting rate of the X-ray telescope during the precession of the satellite axis are shown in a graph.

Ulmer, M. P.↗

Hard X-ray observations of Hercules X-1 by OSO-7.

The X-ray source Her X-1, identified as a pulsating, eclipsing X-ray source, was observed by the UCSD X-ray telescope on the OSO-7 satellite. A three-point spectrum for Her X-1 was determined on the basis of data obtained when the source was in its high-intensity state. Errors in the UCSD result due to uncertainties in the gain and in converting counts per second to photon flux are about 20%.

Ulmer, M. P.↗