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Infrared, radio, and X-ray observations of Cygnus X-3Infrared observations of Cyg X-3 are presented along with X-ray and radio data. A study of the data shows evidence for several types of behavior in the infrared flux variations of Cyg X-3. It is pointed out that a lack of periodic variations observed can be due either to a real absence of these variations or to a masking by an outburst preceding the observation time. There is no simple radio-infrared correlation, although both radio and infrared emissions were observed during the same period of time.
Document ID
19750026708
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Becklin, E. E.
Neugebauer, G.
(Hale Observatories Pasadena, Calif., United States)
Hawkins, F. J.
Mason, K. O.
Sanford, P. W.
(London, University College, Dorking, Surrey, United Kingdom)
Matthews, K.
(California Institute of Technology Pasadena, Calif., United States)
Packman, D.
Schupler, B.
Stark, A.
(Owens Valley Radio Observatory Pasadena, Calif., United States)
Wynn-Williams, C. G.
(Mullard Radio Astronomy Observatory Cambridge, United Kingdom)
Date Acquired
August 8, 2013
Publication Date
September 15, 1974
Publication Information
Publication: Astrophysical Journal
Volume: 192
Subject Category
Astronomy
Accession Number
75A10780
Funding Number(s)
CONTRACT_GRANT: NSF GP-30400X2
CONTRACT_GRANT: NSF GP-35545X
CONTRACT_GRANT: N00014-67-A-0094-0019
CONTRACT_GRANT: NSF GP-23780
CONTRACT_GRANT: NGL-05-002-207
Distribution Limits
Public
Copyright
Other

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