SIMBAD references

2014ApJ...785...94L - Astrophys. J., 785, 94 (2014/April-3)

The lithium abundances of a large sample of red giants.

LIU Y.J., TAN K.F., WANG L., ZHAO G., SATO B., TAKEDA Y. and LI H.N.

Abstract (from CDS):

The lithium abundances for 378 G/K giants are derived with non-local thermodynamic equilibrium correction considered. Among these are 23 stars that host planetary systems. The lithium abundance is investigated, as a function of metallicity, effective temperature, and rotational velocity, as well as the impact of a giant planet on G/K giants. The results show that the lithium abundance is a function of metallicity and effective temperature. The lithium abundance has no correlation with rotational velocity at v sin i < 10 km/s. Giants with planets present lower lithium abundance and slow rotational velocity (v sin i < 4 km/s). Our sample includes three Li-rich G/K giants, 36 Li-normal stars, and 339 Li-depleted stars. The fraction of Li-rich stars in this sample agrees with the general rate of less than 1% in the literature, and the stars that show normal amounts of Li are supposed to possess the same abundance at the current interstellar medium. For the Li-depleted giants, Li-deficiency may have already taken place at the main sequence stage for many intermediate mass (1.5-5 M) G/K giants. Finally, we present the lithium abundance and kinematic parameters for an enlarged sample of 565 giants using a compilation of the literature, and confirm that the lithium abundance is a function of metallicity and effective temperature. With the enlarged sample, we investigate the differences between the lithium abundance in thin-/thick-disk giants, which indicate that the lithium abundance in thick-disk giants is more depleted than that in thin-disk giants.

Abstract Copyright:

Journal keyword(s): methods: data analysis - stars: abundances - stars: late type - techniques: spectroscopic

VizieR on-line data: <Available at CDS (J/ApJ/785/94): table2.dat table5.dat>

Simbad objects: 565

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2019.11.15-22:47:50

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