Possible radio counterpart to IGR J17091-3624

Details Possible radio counterpart to IGR J17091-3624 Possible radio counterpart to IGR J17091-3624

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003atel..152....1r&link_type=abstract

The Astronomer's Telegram, #152

Astronomy and Astrophysics

Astronomy

11

Radio, X-Ray, Gamma Ray, Request For Observations, Transients

Scientific paper

Observations with the Very Large Array (VLA) at 4.9 GHz show a possible radio counterpart to IGR J17091-3624, with a flux density of 1.9+/-0.3 mJy, and a J2000 position of 17 09 02.3 +/- 0.4 - -36 23 33 +/- 5. This is about 80 arcseconds from the INTEGRAL position reported by Kuulkers et al. (ATEL #149), and well within their 3 arcminute error circle. This is the only radio source within that error circle (to the limiting rms noise quoted above).

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