Radio Light Curves of X-ray Sources Obtained with the Green Bank Interferometer

Details Radio Light Curves of X-ray Sources Obtained with the Green Bank Interferometer Radio Light Curves of X-ray Sources Obtained with the Green Bank Interferometer

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...19111017h&link_type=abstract

American Astronomical Society, 191st AAS Meeting, #110.17; Bulletin of the American Astronomical Society, Vol. 29, p.1390

Astronomy and Astrophysics

Astrophysics

Scientific paper

Since November 1996 the Green Bank Inteferometer has been dedicated to 2.25 and 8.3 GHz monitoring of radio emisison from both known and newly discovered X-ray transients, X-ray binaries, active binaries, AGNs, and quasars. This program is funded by the NASA High Energy Astrophysics Program and is intended for radio support of multi-wavelength programs - mainly when satellite observations of high energy X-ray and Gamma-ray sources are involved. This paper summarizes the results for a wide range of sources that have been observed, including GRS 1915+105, Cyg X-3, LSI +61 303, SS433, Sgr A*, Algol, UX Ari, Sco X-1, Cyg X-1, and a number of extra-galactic variable radio sources. In some cases the comparison light curves at radio, soft X-ray (RXTE ASM), and hard X-ray (CGRO BATSE) wavelengths will be presented.

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