Optical Spectroscopy of the IGR J16195-4945 Candidate Counterpart

Details Optical Spectroscopy of the IGR J16195-4945 Candidate Counterpart Optical Spectroscopy of the IGR J16195-4945 Candidate Counterpart

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..804....1t&link_type=abstract

The Astronomer's Telegram, #804

Astronomy and Astrophysics

Astronomy

2

Optical, Binaries, Neutron Stars

Scientific paper

On 2005 October 5, we observed the candidate optical counterpart of the INTEGRAL source IGR J16195-4945 with the EMMI spectrograph attached to the ESO 3.5m NTT in La Silla, Chile (see Tomsick et al. 2006; astro- ph/0603810 v2 and references therein for the details about this likely High-Mass X-ray Binary). The Chandra position of IGR J16195-4945 coincides with the infrared source 2MASS J16193220-4944305 (Ks = 11.00).

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