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Observations of Cosmic X-Ray Sources by the MIT Instrument on the OSO-7∗

Published online by Cambridge University Press:  14 August 2015

G. W. Clark
G. W. Clark*
Affiliation:
Dept. of Physics and Center for Space Research, Massachusetts Institute of Technology, Cambridge, Mass., U.S.A.

Abstract

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The Seventh Orbiting Solar Observatory, OSO-7, carries on board a 1–60 keV X-ray detector for the purpose of measuring the positions, spectra and time variations of X-ray sources. The instrument is described herein, and several topics under investigation and results in publication are mentioned.

Type
Part I: Galactic Sources
Information
Symposium - International Astronomical Union , Volume 55: X- and Gamma-Ray Astronomy , 1973 , pp. 29 - 35
Copyright
Copyright © Reidel 1973 

References

Clark, G. W., Bradt, H. V., Lewin, W. H. G., Markert, T. H., Schnopper, H. W., and Sprott, G. F.: 1972a, Astrophys. J., in press.Google Scholar
Clark, G. W., Bradt, H. V., Lewin, W. H. G., Markert, T. H., Schnopper, H. W., and Sprott, G. F.: 1972b, Astrophys. J. Letters, in press.Google Scholar
Doxsey, R., Murthy, G. T., Rappaport, S., Zaumen, W., and Spencer, J.: 1972, Astrophys. J. Letters 176, L15.Google Scholar
Liller, W.: 1972, IAU Circular 2415 and 2427.Google Scholar