No Radio Emission from IGR J17419-2802 or GRS 1736-297

Details No Radio Emission from IGR J17419-2802 or GRS 1736-297 No Radio Emission from IGR J17419-2802 or GRS 1736-297

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..755....1r&link_type=abstract

The Astronomer's Telegram, #755

Astronomy and Astrophysics

Astronomy

1

Radio, X-Ray, Black Holes, Neutron Stars, Transients

Scientific paper

Pursuant to the report of renewed X-ray activity in IGR J17419-2802 and GRS 1736-297 (ATel #744) on Feb. 19-20, both sources were observed with the Very Large Array (VLA) at 4.86 GHz on Feb. 26. In the case of IGR J17419-2802, there was no source within the revised Swift XRT error circle (ATel #745) with an rms of 95 microJy/beam; the min/max within that error circle were (-0.37, +0.32) mJy/beam.

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