Microquasar Monitoring with the GBI

Details Microquasar Monitoring with the GBI Microquasar Monitoring with the GBI

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.4802w&link_type=abstract

American Astronomical Society, 194th AAS Meeting, #48.02; Bulletin of the American Astronomical Society, Vol. 31, p.893

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Monitoring of the X-ray binaries GRS 1915+105, Cygnus X-3 (2030+407), LSI +61(deg) 303 (0236+610), and SS 433 (1909+048) at 2 and 8 GHz with the Green Bank Interferometer (GBI) is available on the website of the GBI. In addition to the 1997-1999 fluxes which have been available as public domain data, the archival data on these sources prior to 1996 are now included in the archives directory on the GBI website. The GBI is a facility of the NSF, operated by the NRAO with support for the Monitoring Program provided by the US Naval Observatory, the Naval Research Laboratory, and NASA, which should be acknowledged with the requested funding credit statement.

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