Optical counterpart to IGR J16465-4507

Details Optical counterpart to IGR J16465-4507 Optical counterpart to IGR J16465-4507

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..429....1n&link_type=abstract

The Astronomer's Telegram, #429

Astronomy and Astrophysics

Astronomy

20

Optical, Binaries, Neutron Stars, Transients

Scientific paper

Intermediate resolution spectra of the only star in the XMM-Newton error box for IGR J16465-4507 (ATel #329, #336), USNO-B1.0 0448-00520455 = 2MASS J16463526-4507045, have been taken with the 3.5-m NTT, in La Silla (ESO proposal 274.D-0510). As anticipated in ATel #338, the star is a reddened early-type supergiant and hence certainly the correct counterpart. The spectral type is estimated at B0.5I.

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