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Searches for correlated X-ray and radio emission from X-ray burst sourcesThe NRAO Green Bank interferometer has been used to monitor MXB 1730-335 and MXB 1837+05 during periods when 68 X-ray bursts were detected by X-ray observations. No significant radio emission was detected from these objects, or from MXB 1820-30 and MXB 1906+00, which emitted no bursts throughout the simultaneous observations. The data place upper limits on radio emission from these objects in the 2695 and 8085 MHz bands.
Document ID
19780053747
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Johnson, H. M.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Catura, R. C.
(Lockheed Research Laboratories Palo Alto, Calif., United States)
Lamb, P. A.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
White, N. E.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Sanford, P. W.
(London, University College, Mullard Space Science Laboratory, Dorking, Surrey, United Kingdom)
Hoffman, J. A.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Lewin, W. H. G.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Jernigan, J. G.
(MIT Cambridge, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
June 1, 1978
Publication Information
Publication: Astrophysical Journal
Subject Category
Astronomy
Accession Number
78A37656
Funding Number(s)
CONTRACT_GRANT: NAS5-23570
CONTRACT_GRANT: NAS5-11450
Distribution Limits
Public
Copyright
Other

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