Large-scale Jets in GRS 1915+105

Details Large-scale Jets in GRS 1915+105 Large-scale Jets in GRS 1915+105

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..503....1r&link_type=abstract

The Astronomer's Telegram, #503

Astronomy and Astrophysics

Astronomy

Radio, Millimeter, Sub-Millimeter, Infra-Red, Optical, X-Ray, Binaries, Black Holes, Transients, Variables

Scientific paper

Observations with the Very Large Array (VLA), originally intended to support the HERO balloon flight, show multiple arcsecond-scale components moving out from the core of the black hole X-ray binary GRS 1915+105. Data taken at 8.46 GHz on May 11 and May 23 show extended emission along the known jet axis of this microquasar (e.g., Mirabel & Rodriguez 1994 [MR94], Nature, 371, 46-48). The beam was roughly round in both observations, with a full-width at half-maximum of about 0.67 arcseconds.

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