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HD 181068: a triply eclipsing system with intrinsically variable red giant component

Derekas, A. and Borkovits, T. and Fuller, J. and Huber, D. and Lehmann, H. (2014) HD 181068: a triply eclipsing system with intrinsically variable red giant component. In: Setting a New Standard in the Analysis of Binary Stars. EAS Publications Series. No.64. EDP Sciences , Les Ulis, France, pp. 343-350. ISBN 978-2-7598-1161-8. http://resolver.caltech.edu/CaltechAUTHORS:20190425-152212177

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Abstract

We present the analysis of HD 181068 which is one of the first triply eclipsing triple system discovered. Using Kepler photometry, ground based spectroscopic and interferometric measurements, we determined the stellar and orbital parameters of the system. We show that the oscillations observed in the red giant component of the system are tidally forced oscillations, while one of the most surprising results is that it does not show solar-like oscillations.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1051/eas/1364048DOIArticle
ORCID:
AuthorORCID
Derekas, A.0000-0002-6526-9444
Borkovits, T.0000-0002-8806-496X
Fuller, J.0000-0002-4544-0750
Huber, D.0000-0001-8832-4488
Additional Information:© EAS, EDP Sciences, 2014.
Record Number:CaltechAUTHORS:20190425-152212177
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190425-152212177
Official Citation:HD 181068: a triply eclipsing system with intrinsically variable red giant component A. Derekas, T. Borkovits, J. Fuller, D. Huber and H. Lehmann EAS Publications Series, 64 (2013) 343-350 DOI: https://doi.org/10.1051/eas/1364048
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:94982
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:26 Apr 2019 17:37
Last Modified:26 Apr 2019 17:37

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