ATCA detection of increased radio emission from XTE J1752-223

Details ATCA detection of increased radio emission from XTE J1752-223 ATCA detection of increased radio emission from XTE J1752-223

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2400....1b&link_type=abstract

The Astronomer's Telegram, #2400

Astronomy and Astrophysics

Astronomy

5

Radio, Request For Observations, Binaries, Black Holes, Transients

Scientific paper

Following the announcement that the new X-ray transient source, XTE J1752-223 (ATel. 2258), is making a transition from the hard to the intermediate state (ATel. 2387, 2391, 2396), we have observed the radio counterpart with the Australia Telescope Compact Array and the new CABB back-end. The radio source has risen from the previous ~2 mJy plateau to 20 mJy at 1.2, 2.5, 5.5, 9, 17, 19 GHz on January 21.

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