Galactic chemical evolution of exoplanet host stars: Are high-mass planetary systems young?
Galactic chemical evolution of exoplanet host stars: Are high-mass planetary systems young?
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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
The imprints of stellar nucleosynthesis and chemical evolution of the galaxy can be seen in different stellar populations, with older generation stars showing higher \(\alpha\)-element abundances while the later generations becoming enriched with iron-peak elements. The evolutionary connections and chemical characteristics of circumstellar disks, s...
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Full title
Galactic chemical evolution of exoplanet host stars: Are high-mass planetary systems young?
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TN_cdi_proquest_journals_2672172545
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2672172545
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2205.15793
