On the link between rotation, chromospheric activity and Li abundance in subgiant stars
classification
🌌 astro-ph
keywords
abundancestarssubgiantactivityanalyzedbonachromosphericcode
read the original abstract
The connection rotation-CaII emission flux-lithium abundance is analyzed for a sample of bona fide subgiant stars, with evolutionary status determined from HIPPARCOS trigonometric parallax measurements and from the Toulouse-Geneva code.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.