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Characterizing binary properties of 5 m⊙ stars: new approaches using cepheids

Published online by Cambridge University Press:  25 February 2014

N.R. Evans
N.R. Evans*
Affiliation:
SAO, MS 4, 60 Garden St., Cambridge, MA 02138, USA
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Abstract

Cepheids provide approaches to determining binary parameters which are often complementary to those for main sequence massive and intermediate mass stars. Specifically, we are using high resolution imaging, radial velocities, and X-ray studies to determine binary characteristics. Among the results are that they have both a high frequency of binary systems, and also a high proportion of triple systems.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 64: Setting a New Standard in the Analysis of Binary Stars , 2013 , pp. 81 - 84
Copyright
© EAS, EDP Sciences, 2014

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References

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