Binaries among low-mass stars in nearby young moving groups
Binaries among low-mass stars in nearby young moving groups
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Ithaca: Cornell University Library, arXiv.org
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Language
English
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Ithaca: Cornell University Library, arXiv.org
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Contents
The solar galactic neighbourhood contains a number of young co-moving associations of stars (so-called `young moving groups') with ages of ~10--150 Myr, which are prime targets for a range of scientific studies, including direct imaging planet searches. The late-type stellar population of such groups still remain in their pre-main sequence phase, a...
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Full title
Binaries among low-mass stars in nearby young moving groups
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TN_cdi_proquest_journals_2074686524
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2074686524
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1612.02443
