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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 st...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2082542361

Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tau

About this item

Full title

Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tau

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2015-04

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

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...

Alternative Titles

Full title

Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tau

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2082542361

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2082542361

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1503.04435

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