Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.187..299t&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 187, Apr. 1979, p. 299-302. Research supported by the Australian Resear
Astronomy and Astrophysics
Astronomy
2
Radio Bursts, Radio Sources (Astronomy), Satellite Observation, Spaceborne Astronomy, X Ray Sources, Radiant Flux Density, Radio Astronomy, Radio Telescopes, Sas-3, Spaceborne Telescopes, X Ray Astronomy
Scientific paper
On June 17, 1977, the X-ray burst source MXB 1636-53 was simultaneously monitored for about 4 hr with the Parkes 64-m radio telescope at a frequency of 14.7 GHz and the SAS 3 X-ray satellite (1.3-12 keV). One X-ray burst was observed; an upper limit (2 sigmas) of 200 mJy is reported for any radio burst coincident with the X-ray event. During the X-ray burst the radio/X-ray time-integrated flux ratio was no more than 375 with a 90 percent confidence. An upper limit (2 sigmas) of 22 mJy was determined for any steady 14.7-GHz source coincident with the X-ray position.
Doty John
Duldig Marc L.
Haynes Raymond F.
Hoffman Anthony J.
Lewin Walter H. G.
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