Variable radio source GT0116+622 is a possible counterpart to CAS Gamma-1

Details Variable radio source GT0116+622 is a possible counterpart to CAS Gamma-1 Variable radio source GT0116+622 is a possible counterpart to CAS Gamma-1

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986natur.323..602g&link_type=abstract

Nature (ISSN 0028-0836), vol. 323, Oct. 16, 1986, p. 602, 603. NSERC-supported research.

Astronomy and Astrophysics

Astronomy

6

Gamma Ray Astronomy, Radio Sources (Astronomy), X Ray Binaries, Astronomical Coordinates, Radiant Flux Density, Radio Emission, Sky Surveys (Astronomy), Variable Stars

Scientific paper

The authors report the discovery of a highly variable radio source which coincides in position with the transient TeV γ-ray source Cas γ-1. They have obtained an accurate radio position with the VLA telescope but no optical counterpart was found on the Mount Palomar Sky Survey prints. The authors have also obtained upper limits on radio emission from the binary X-ray pulsar, 4U 0115+634, another proposed identification for Cas γ-1.

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