Marginally low mass ratio close binary system V1191 Cyg
Marginally low mass ratio close binary system V1191 Cyg
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Ithaca: Cornell University Library, arXiv.org
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Contents
In this study, we present photometric and spectroscopic variations of the extremely small mass ratio (\(q\simeq 0.1\)) late-type contact binary system \astrobj{V1191 Cyg}. The parameters for the hot and cooler companions have been determined as \(M_\textrm{h}\) = 0.13 (1) \(M_{\odot}\), \(M_\textrm{c}\) = 1.29 (8) \(M_{\odot}\), \(R_\textrm{h}\) =...
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Full title
Marginally low mass ratio close binary system V1191 Cyg
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Record Identifier
TN_cdi_proquest_journals_2086848244
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2086848244
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1107.0277
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