Abundances of evolved stars
收藏B2FIND2026-04-04 收录
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https://b2find.eudat.eu/dataset/7d5a6971-fe5a-5e96-9696-9157c12e0496
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Currently, the core accretion model has its strongest observational evidence on the chemical signature of mostly main sequence stars with planets. We aim to test whether the...
