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Results of X-ray and optical monitoring of Scorpius X-1 in 1970Scorpius X-1 was monitored at optical and X-ray wavelengths from 1970 April 26 to 1970 May 20. The optical observations were made at six observatories around the world, and the X-ray observations were made by the Vela satellites. There was a tendency for the object to show greater variability in X-ray emission when the object was optically bright. The intensity histograms for both the optical and X-ray observations are discussed, as well as periodic variations in the optical intensity.
Document ID
19750045668
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Mook, D. E.
Messina, R. J.
(Dartmouth College Hanover, N.H., United States)
Hiltner, W. A.
(Michigan, University Ann Arbor, Mich., United States)
Belian, R.
Conner, J.
Evans, W. D.
Strong, I.
(California, University Los Alamos, N. Mex., United States)
Blanco, V. M.
Hesser, J. E.
Kunkel, W. E.
(Observatorio Interamericano de Cerro Tololo La Serena, Chile)
Date Acquired
August 8, 2013
Publication Date
April 15, 1975
Publication Information
Publication: Astrophysical Journal
Volume: 197
Subject Category
Astronomy
Accession Number
75A29740
Funding Number(s)
CONTRACT_GRANT: NGR-23-005-464
Distribution Limits
Public
Copyright
Other

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