H1743-322 re-appears

Details H1743-322 re-appears H1743-322 re-appears

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..575....1r&link_type=abstract

The Astronomer's Telegram, #575

Astronomy and Astrophysics

Astronomy

8

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

Scientific paper

Very Large Array (VLA) observations of the black hole candidate binary H1743-322 = IGR J1746-3213 = XTE J17464-3213 (e.g., ATel #301, #314) show that the central radio source has re-appeared. Data taken on August 7, 2005 (MJD 53589.25) at 4.86 GHz gave a clear detection with a flux density of 0.59 +/- 0.07 mJy; data taken at the same frequency on June 11 (MJD 53532.30) gave only an upper limit, with a nominal flux density at the source position of 0.03 +/- 0.04 mJy/beam.

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