IGR/XTE J17464-3213: New radio position and optical counterpart

Details IGR/XTE J17464-3213: New radio position and optical counterpart IGR/XTE J17464-3213: New radio position and optical counterpart

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003atel..146....1s&link_type=abstract

The Astronomer's Telegram, #146

Astronomy and Astrophysics

Astronomy

15

Radio, Infra-Red, Optical, X-Ray, Gamma Ray, Request For Observations, Black Holes, Transients

Scientific paper

Taking into account all VLA observations of this source up to April 8, we have obtained a revised radio position for IGR/XTE J17464-3213; 17 46 15.608 +/- 0.17" -32 14 00.6 +/- 0.5" (J2000) This is 0.7" south of the position reported in IAUC 8105 bringing the VLA position closer to a nearby optical counterpart present in Magellan I and R-band images (ATEL #141). This possible counterpart is consistent with the K-band source reported by Baba et al.

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