SIMBAD references

2019ApJS..245...33G - Astrophys. J., Suppl. Ser., 245, 33-33 (2019/December-0)

Lithium-rich giants in LAMOST survey. I. The catalog.

GAO Q., SHI J.-R., YAN H.-L., YAN T.-S., XIANG M.-S., ZHOU Y.-T., LI C.-Q. and ZHAO G.

Abstract (from CDS):

Standard stellar evolution model predicts a severe depletion of lithium (Li) abundance during the first dredge up process (FDU). Yet a small fraction of giant stars are still found to preserve a considerable amount of Li in their atmospheres after the FDU. Those giants are usually identified as Li-rich by a widely used criterion, A(Li) > 1.5 dex. A large number of works dedicated to searching for and investigating this minority of the giant family, and the amount of Li-rich giants, has been largely expanded on, especially in the era of big data. In this paper, we present a catalog of Li-rich giants found from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) survey with Li abundances derived from a template-matching method developed for LAMOST low-resolution spectra. The catalog contains 10,535 Li-rich giants with Li abundances from ∼1.5 to ∼4.9 dex. We also confirm that the ratio of Li-rich phenomenon among giant stars is about 1%-or more specifically, 1.29%-from our statistically important sample. This is the largest Li-rich giant sample ever reported to date, which significantly exceeds amount of all reported Li-rich giants combined. The catalog will help the community to better understand the Li-rich phenomenon in giant stars.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): Late stellar evolution - Stellar abundances - Late-type giant stars - Chemically peculiar stars

Status at CDS:   being processed
// Tables of objects will be appraised for possible ingestion in SIMBAD.

Simbad objects: 35

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2019ApJS..245...33G and select 'bookmark this link' or equivalent in the popup menu


2020.03.31-19:50:57

© Université de Strasbourg/CNRS

    • Contact