Renewed radio emission from GRO J1655-40

Details Renewed radio emission from GRO J1655-40 Renewed radio emission from GRO J1655-40

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..443....1r&link_type=abstract

The Astronomer's Telegram, #443

Astronomy and Astrophysics

Astronomy

3

Radio, Binaries, Black Holes, Transients

Scientific paper

The radio counterpart to the black hole X-ray binary GRO J1655-40 has again re-appeared, and is growing stronger (cf. ATEL #441). Observations taken at 4.86 GHz with the Very Large Array (VLA) showed a 1.77 +/- 0.07 mJy source on March 16th (13:38 to 14:29 UT), and a 3.6 +/- 0.1 mJy source on March 18th (12:59 to 13:10 UT). The latter represents the strongest radio emission so far during the current outburst.

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