Host star metallicity of directly imaged wide-orbit planets: implications for planet formation
Host star metallicity of directly imaged wide-orbit planets: implications for planet formation
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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
Directly imaged planets are self-luminous companions of pre-main sequence and young main sequence stars. They reside in wider orbits (\(\sim10\mathrm{s}-1000\mathrm{s}\)~AU) and generally are more massive compared to the close-in (\(\lesssim 10\)~AU) planets. Determining the host star properties of these outstretched planetary systems is important...
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Full title
Host star metallicity of directly imaged wide-orbit planets: implications for planet formation
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TN_cdi_proquest_journals_2473575287
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2473575287
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2012.13694
