Titlebook: Explaining Lithium Enriched Red Giant Branch Stars; Claudia Aguilera-Gómez Book 2018 Springer Nature Switzerland AG 2018 lithium red giant

dissolution

Abutment

External Mechanismsce of Li. This light element, sometimes used to distinguish brown dwarfs from low-mass stars, is burned in objects with masses higher than . ∼ 0.065 M.. The ingestion of this kind of objects could increase the superficial Li abundance of the star.

arsenal

Trumpler 20have broadly the same mass, so Li-enriched stars are easier to identify. In this chapter, we analyze the Li abundance pattern of the open cluster Trumpler 20, as published by the Gaia-ESO Survey, and identify 2 enriched giants, which could have experienced planet engulfment.

吹牛大王

漂浮

Summary and Future Workr the Big Bang, and it is also used extensively as a proxy for mixing inside stars, being very sensitive to environmental conditions. Although it is produced inside stars by nuclear burning, it is rapidly burned by proton capture inside low-mass stars during the main sequence. When the star enters i

dry-eye

Book 2018he stars in question grew in size while becoming giants. She shows that this process is indeed able to explain an important fraction of giants with Li levels above the three times solar threshold, but that some other mechanism is needed to explain the remaining fraction. While this is an important d

Glaci冰

output

2190-5053 deed able to explain an important fraction of giants with Li levels above the three times solar threshold, but that some other mechanism is needed to explain the remaining fraction. While this is an important d978-3-030-02583-0Series ISSN 2190-5053 Series E-ISSN 2190-5061

弯曲道理

tolerance