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Characterizing New Eclipsing Binaries Identified from STEREO Photometry

Published online by Cambridge University Press:  23 April 2012

Harry Markov ,
Zlatan Tsvetanov ,
Ilian Iliev ,
Ivanka Stateva  and
Nevena Markova
Harry Markov
Affiliation:
Institut of Astronomy and National Astronomical Observatory Rozhen, Bulgaria
Zlatan Tsvetanov
Affiliation:
Johns Hopkins University, Department of Physics and Astronomy, USA email: hmarkov@astro.bas.bg
Ilian Iliev
Affiliation:
Institut of Astronomy and National Astronomical Observatory Rozhen, Bulgaria
Ivanka Stateva
Affiliation:
Institut of Astronomy and National Astronomical Observatory Rozhen, Bulgaria
Nevena Markova
Affiliation:
Institut of Astronomy and National Astronomical Observatory Rozhen, Bulgaria
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Abstract

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Since 2010, a program to explore new eclipsing binary systems identified from STEREO photometry has been in progress. Our first results are presented here: light curves and high resolution spectra taken with Coudé spectrograph (National Astronomical Observatory Rozhen) and ARC Échelle spectrometer (ARCES, Apache Point Observatory).

Keywords

techniques: radial velocitiesphotometricspectroscopic; binaries: eclipsing

References

Griffin, R. F. 2006, Observatory, 126, 1Google Scholar
Montes, D., Martin, E. L., Fernandez-Figueroa, M. J., et al. , 1997, A&AS, 123, 473Google Scholar
Wright, K. T. et al. , 2011, arXiv:1103.0911Google Scholar