HD 306414, the Optical Counterpart to the Peculiar X-Ray Transient IGR J11215-5952

Details HD 306414, the Optical Counterpart to the Peculiar X-Ray Transient IGR J11215-5952 HD 306414, the Optical Counterpart to the Peculiar X-Ray Transient IGR J11215-5952

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..422..259l&link_type=abstract

High Energy Phenomena in Massive Stars ASP Conference Series, Vol. 422, proceedings of a conference held 2-5 February 2009 in Ja

Astronomy and Astrophysics

Astronomy

1

Scientific paper

HD 306414 is the optical counterpart to the transient X-ray source IGR J11215-5952, characterised by short flares occurring every 165 days. In order to improve our understanding of this source, we obtained high-resolution spectroscopy of HD 306414 around the time of the February 2007 X-ray outburst. Large variations in the shape of the Hα emission feature and the radial velocities of metallic lines are seen around the time of the X-ray emission.

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