Clarification on the association between IGR J17464-3213 and H1743-322

Details Clarification on the association between IGR J17464-3213 and H1743-322 Clarification on the association between IGR J17464-3213 and H1743-322

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003atel..136....1m&link_type=abstract

The Astronomer's Telegram, #136

Astronomy and Astrophysics

Astronomy

16

X-Ray, A Comment, Binaries, Black Holes, Transients

Scientific paper

In ATEL #133, we commented that newly reported INTEGRAL transient IGR J17464-3213 (ATEL #132) may be HEAO source H1743-322 (also known as H1741-322). The most commonly known position for H1743-322 is taken from the HEAO A-1 catalog (Wood et al. 1984, ApJS, 56, 507). However, there are in fact two candidate positions for the source, as determined by the HEAO A-3 instrument (Gursky et al. 1978, ApJ, 223, 973), both equally likely.

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