Precise mass and radius measurements for the components of the bright solar-type eclipsing binary st...
Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tau
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
V1094 Tau is bright eclipsing binary star with an orbital period close to 9 days containing two stars similar to the Sun. Our aim is to test models of Sun-like stars using precise and accurate mass and radius measurements for both stars in V1094 Tau. We present new spectroscopy of V1094 Tau which we use to estimate the effective temperatures of bot...
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Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tau
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TN_cdi_proquest_journals_2082542361
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2082542361
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1503.04435