GRO J1655-40 radio counterpart fades

Details GRO J1655-40 radio counterpart fades GRO J1655-40 radio counterpart fades

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..441....1r&link_type=abstract

The Astronomer's Telegram, #441

Astronomy and Astrophysics

Astronomy

7

Radio, Binaries, Black Holes, Transients

Scientific paper

The radio counterpart to the black hole X-ray binary GRO J1655-40 has faded considerably over the past few days. Observations by the Very Large Array (VLA) taken on March 14th, from 12:25 to 12:35 UT, gave no detection, with a nominal flux density at the location of the source of 0.15 +/- 0.14 mJy/beam at 8.46 GHz. The full radio light curve is shown at:

http://www.aoc.nrao.edu/~mrupen/XRT/GRJ1655-40/grj1655 -40.shtml This radio cutoff corresponds to the X-ray rise and softening reported in ATEL #440.

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