The likely optical counterpart to the X-ray transient IGR J01363+6610 (Resubmission of ATel#339)

Details The likely optical counterpart to the X-ray transient IGR J01363+6610 (Resubmission of ATel#339) The likely optical counterpart to the X-ray transient IGR J01363+6610 (Resubmission of ATel#339)

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..343....1r&link_type=abstract

The Astronomer's Telegram, #343

Astronomy and Astrophysics

Astronomy

3

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

Scientific paper

After the submission of ATel #339 a few formatting inconsistencies and some missing/incorrect information were spotted. This is the corrected version of ATel #339. It also contains new information concerning the association of the proposed counterpart with the Halpha emission line star [KW97] 6-30. We report photometric and spectroscopic optical observations of the likely optical counterpart to the X-ray transient IGR J01363+6610 discovered by INTEGRAL (Grebenev et al., ATel #275).

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