Detection of Probable Jet Component to XTE J1752-233 with the e-EVN

Details Detection of Probable Jet Component to XTE J1752-233 with the e-EVN Detection of Probable Jet Component to XTE J1752-233 with the e-EVN

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2438....1b&link_type=abstract

The Astronomer's Telegram, #2438

Astronomy and Astrophysics

Astronomy

3

Radio, Binaries, Black Holes, Transients

Scientific paper

Following the reported increased radio emission of XTE J1752-233 (ATel. 2400) during its X-ray spectral softening (ATel. 2387, 2391, 2396), we have made an additional radio observation with the European VLBI Network (EVN) in real-time e-VLBI mode. A 2-hour observation on 2010 February 11 detected an 8-sigma source at 5 GHz with coordinates RA 17 52 15.064, Dec. -22 30 31.982 (to uncertainty ~2 mas).

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