Hard X-Ray Observations of Hercules X-1 by OSO-7
Melville P. Ulmer, William A. Baity, W. A. Wheaton, Leif E. Peterson
Abstract
Melville P. Ulmer, William A. Baity, W. A. Wheaton, Leif E. Peterson
Abstract
The UCSD X-ray telescope on the oSO-7 scanned the periodic variable X-ray source Her X-1 from 1972 May 30 to 1972 June 1. Analysis of the quick-look data in the 7-26 keV range shows low intensity at 12 2 hours UT, 1972 May 31, which is ezpected from the previously determined 1.7-day period. The source was observed in its high-intensity state 30 hours earlier than predicted from the Uhitru determination of the s5.7-day period and its phase. The spectrum over the 240 keV range in the high-intensity state can be fitted by 0.2S/E'. photons (cm2 5 kev) 1
OpenAlex reports 14 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
The UCSD X-ray telescope on the oSO-7 scanned the periodic variable X-ray source Her X-1 from 1972 May 30 to 1972 June 1. Analysis of the quick-look data in the 7-26 keV range shows low intensity at 12 2 hours UT, 1972 May 31, which is ezpected from the previously determined 1.7-day period. The source was observed in its high-intensity state 30 hours earlier than predicted from the Uhitru determination of the s5.7-day period and its phase. The spectrum over the 240 keV range in the high-intensity state can be fitted by 0.2S/E'. photons (cm2 5 kev) 1
Key concepts: Physics, Astrophysics, X-ray, Intensity (physics), Telescope, Astronomy, Optics