The spectral type of the optical counterpart to the high-mass X-ray binary IGR J06074+2205

Details The spectral type of the optical counterpart to the high-mass X-ray binary IGR J06074+2205 The spectral type of the optical counterpart to the high-mass X-ray binary IGR J06074+2205

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2085....1r&link_type=abstract

The Astronomer's Telegram, #2085

Astronomy and Astrophysics

Astronomy

1

Optical, Binaries, Neutron Stars

Scientific paper

Spectroscopic observations of the optical counterpart to the high- mass X-ray binary IGR J06074+2205 were obtained from the 1.3m telescope of the Skinakas observatory in Crete (Greece) and from the 1.5m telescope of the Fred Lawrence Whipple Observatory at Mt. Hopkins (Arizona) on several occasions throughout 2006-2008.These observations allowed us to identify the spectral type of this source and study its long-term spectral variability.

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