Lithium evolution in the Galactic thin disc from Main-Sequence and early Red-Giant-Branch stars
C. T. Nguyen, G. Cescutti, F. Matteucci, F. Rizzuti, A. Mucciarelli, D. Romano, L. Magrini, A. J. Korn, A. Bressan, and L. Girardi

TL;DR
This study models lithium evolution in the galactic thin disc, incorporating nova contributions and stellar depletion, and confirms the existence of two lithium abundance plateaus in stars, supporting novae as key lithium sources.
Contribution
It introduces the first analysis including early RGB stars and constrains nova lithium yields within chemical evolution models.
Findings
Confirmation of a second lithium plateau in early RGB stars.
Best-fit nova lithium yield of 2.34×10⁻⁵ M☉ per nova.
Support for novae as primary galactic lithium producers.
Abstract
The role of novae as producers of galactic lithium has been suggested since the 1970s, and it has been reconsidered recently with the detection of Be in their outbursts. At the same time, stellar models are moving forward to comprehend the discrepancy between the primordial lithium abundance predicted by the standard Big Bang Nucleosynthesis theory and the measured value of old dwarf stars. In this work, we follow the evolution of Li in the galactic thin disc starting from a primordial value of A(Li)=2.69 dex and applying Li depletion corrections of the stellar model with overshooting to our chemical evolution models. We use the upper envelope of the observational data to constrain the models. In addition to the dwarf main sequence (MS) stars, our analysis includes, for the first time, the early red-giant-branch (RGB) stars. Besides the renowned Spite plateau of the MS stars…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
