The correct optical counterpart to IGR J11435-6109

Details The correct optical counterpart to IGR J11435-6109 The correct optical counterpart to IGR J11435-6109

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1239....1n&link_type=abstract

The Astronomer's Telegram, #1239

Astronomy and Astrophysics

Astronomy

2

Optical, X-Ray, Binaries, Neutron Stars, Pulsars, Stars

Scientific paper

Even though an initial analysis (ATel #370) suggested that the Be star USNO-B1.0 0288-0337948 was the likely counterpart to the 162-s X-ray pulsar IGR J11435-6109 (ATel #350, #362), a deeper search of the error circle using the method described in Negueruela & Schurch (2007, A&A 461, 631) detected a fainter candidate emission-line object, namely 2MASS J11440030-6107364 = USNO-B1.0 0288-0337502, which has been confirmed as the correct counterpart by a Chandra localisation (ATel #1231).

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