A long-term radio study of Hercules X-1

Details A long-term radio study of Hercules X-1 A long-term radio study of Hercules X-1

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193p..35c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 193, Nov. 1980, p. 35P-37P.

Astronomy and Astrophysics

Astronomy

1

Binary Stars, Radio Sources (Astronomy), Variable Stars, X Ray Sources, Radio Emission, Stellar Radiation

Scientific paper

The pulsating X-ray binary system Hercules X-1 has been studied at 4.76 GHz for 35 days using the NRAO 300-ft radio telescope. At no time was any emission detected and an upper limit of 2 mJy was found for any emission in phase with the 35-day X-ray cycle. This result, combined with other observations, suggests that pulsating X-ray binary systems, unlike nonpulsating systems, are probably not radio sources.

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