Lithium-rich Giants in LAMOST Survey. I. The Catalog
arXiv:1912.08431 · doi:10.3847/1538-4365/ab505c
Abstract
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 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.
References in corpus (34)
- The First Data Release (DR1) of the LAMOST general survey
- Thermohaline instability and rotation-induced mixing. I - Low- and intermediate-mass solar metallicity stars up to the end of the AGB
- The accretion of planets and brown dwarfs by giant stars -- II. solar mass stars on the red giant branch
- Signatures of intrinsic Li depletion and Li-Na anti-correlation in the metal-poor globular cluster NGC6397
- The LAMOST Stellar Parameter Pipeline at Peking University --- LSP3
- Origin of lithium enrichment in K giants
- The K giant stars from the LAMOST survey data I: identification, metallicity, and distance
- Tidal interactions between binary stars drives lithium production in low-mass red giants
- Metal-Poor Lithium-Rich Giants in the Radial Velocity Experiment Survey
- Lithium-Rich Giants in Globular Clusters
- Lithium-Rich Field Giants in the Sloan Digital Sky Survey
- Old puzzle, new insights: a lithium rich giant quietly burning helium in its core
- Lithium-rich giants in the Galactic thick disk
- The nature of the Li enrichment in the most Li-rich giant star
- The lithium abundances for a large sample of red giants
- The Li-age correlation: the Sun is unusually Li deficient for its age
- BD+48 740 - Li overabundant giant star with a planet. A case of recent engulfment?
- Three Li-rich K giants: IRAS 12327-6523, IRAS 13539-4153, and IRAS 17596-3952
- Li-rich RGB stars in the Galactic Bulge
- Survey of Li-rich giants among Kepler and LAMOST fields: Determination of Li-rich giants Evolutionary Phase
- The Penn State - Torun Centre for Astronomy Planet Search stars. II. Lithium abundance analysis of the Red Giant Clump sample
- Enormous Li-enhancement preceding red giant phases in low-mass stars in the Milky Way halo
- A Lithium-Rich Red Giant Below the Clump in the Kepler Cluster, NGC 6819
- Study of Lithium Rich Giants with the GALAH Spectroscopic Survey
- Lithium abundances along the RGB: FLAMES-GIRAFFE spectra of a large sample of low-mass Bulge stars
- Li evolution in the thin and thick disks of the Milky Way
- Discovery of Super-Li Rich Red Giants in Dwarf Spheroidal Galaxies
- The Gaia -ESO Survey: Lithium enrichment histories of the Galactic thick and thin disc
- The Gaia-ESO Survey: properties of newly discovered Li-rich giants
- Two new Super Li-rich core He-burning giants: A new twist to the long tale of Li enhancement in K giants
- Spectroscopic study of two new super Li rich red clump K giants
- High-resolution spectroscopic analysis of a large sample of Li-rich giants found by LAMOST
- Super lithium-rich K giant with low to ratio
- A Search for Candidate Li-Rich Giant Stars in SDSS DR10
Cited by in corpus (37)
- Overview of the LAMOST survey in the first decade
- Most Lithium-rich Low-mass Evolved Stars Revealed as Red Clump stars by Asteroseismology and Spectroscopy
- Lithium Enrichment Signatures of Planetary Engulfment Events in Evolved Stars
- Light Elements in the Universe
- The Gaia-ESO Survey: Calibrating the lithium-age relation with open clusters and associations. I. Cluster age range and initial membership selections
- Data mining techniques on astronomical spectra data. II : Classification Analysis
- Lithium and Beryllium in the Gaia-Enceladus Galaxy
- Search for lithium-rich giants in 32 open clusters with high-resolution spectroscopy
- WIYN Open Cluster Study: The Old Open Cluster, NGC 188, and a Re-evaluation of Lithium-Richness Among Red Giants
- On the Chemical and Kinematic Consistency Between N-rich Metal-poor Field Stars and Enriched Populations in Globular Clusters
- Many Roads Lead to Lithium: Formation Pathways For Lithium-Rich Red Giants
- Hydrodynamics and survivability during post-main-sequence planetary engulfment
- Mass Matters: No Evidence for Ubiquitous Lithium Production in Low-Mass Clump Giants
- The Lithium Abundances from the Large Sky Area Multi-object Fiber Spectroscopic Telescope Medium-resolution Survey. I. The Method
- Evidence of extra-mixing in field giants as traced by lithium and carbon isotope ratio
- Lithium Evolution of Giant Stars Observed by LAMOST and Kepler
- The Gaia-ESO Survey: Preparing the ground for 4MOST & WEAVE galactic surveys. Chemical evolution of lithium with machine learning
- WIYN Open Cluster Study LXXXV. Li in NGC 2243 -- Implications for Stellar and Galactic Evolution
- Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT
- Li-rich Giants in LAMOST Survey. III. The statistical analysis of Li-rich giants
- Lithium in red giants: the roles of the He-core flash and the luminosity bump
- Li-rich and super Li-rich giants produced by element diffusion
- An unsupervised method for identifying -enriched stars directly from spectra: Li in LAMOST
- Searching for r-process-enhanced stars in the LAMOST Survey I: The Method
- Lithium in Kepler Red Giants: Defining Normal and Anomalous
- Signature of a massive rotating metal-poor star imprinted in the Phoenix stellar stream
- Li-rich Giants Identified from LAMOST DR8 Low-Resolution Survey
- Hot Jupiter engulfment by a red giant in 3D hydrodynamics
- Distribution and evolution of Li abundance in red clump stars can be explained by the internal gravity waves
- The enigma of Li-rich giants and its relation with temporal variations observed in radial velocity and stellar activity signals
- LAMOST/HRS Spectroscopic Analysis of Two New Li-rich Giants
- Convective Mixing: The Formation Channel of Li-rich Giants
- The true nature of HE0057-5959, the most metal-poor Li-rich star
- Discovery of a Metal-Poor Red Giant Star with the Highest Ultra-Lithium Enhancement
- Lithium evolution in the Galactic thin disc from Main-Sequence and early Red-Giant-Branch stars
- WIYN Open Cluster Study LXXXI. Caught in the Act? The Peculiar Red Giant NGC 2243-W2135
- The highest mass Kepler red giants -- II. Spectroscopic parameters, the amplitude-activity relation, and unexpected halo orbits