The G+M eclipsing binary V530 Orionis: A stringent test of magnetic stellar evolution models for low...
The G+M eclipsing binary V530 Orionis: A stringent test of magnetic stellar evolution models for low-mass stars
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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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We report extensive photometric and spectroscopic observations of the 6.1-day period, G+M-type detached double-lined eclipsing binary V530 Ori, an important new benchmark system for testing stellar evolution models for low-mass stars. We determine accurate masses and radii for the components with errors of 0.7% and 1.3%, as follows: M(A) = 1.0038 +...
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The G+M eclipsing binary V530 Orionis: A stringent test of magnetic stellar evolution models for low-mass stars
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TN_cdi_proquest_journals_2083002841
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2083002841
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2331-8422
DOI
10.48550/arxiv.1410.6170
