Spectroscopic study of two new super Li-rich red clump K giants. Issue 3 (30th October 2018)

• Record Type: Journal Article
• Authors: Singh, Raghubar; Reddy, Bacham E; Kumar, Yerra Bharat
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 482:Issue 3(2019)
• Page Start: 3822
• Page End: 3830
• Publication Date: 2018-10-30
• Subjects: stars: abundances -- stars: atmospheres -- stars: fundamental parameters -- stars: interiors -- stars: low-mass; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/sty2939
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: In this paper, we report the discovery of two new super Li-rich K giants: HD 24960 and TYC 1751-1713-1. Based on high-resolution ( R ≈ 60 000) spectroscopy, we have derived Li abundance of A (Li) ≈ 4.0 dex for both stars. Other elemental abundances are normal of typical K giants. Low ratios of [C/N] ≤ −0.25 and 12 C/ 13 C ≤ 10 suggest that the stars are in the upper red giant branch (RGB) phase. Further, based on Gaia astrometry and secondary calibrations using Kepler asteroseismic and LAMOST spectroscopic data, we argue that both stars belong to the red clump (RC) phase with core He burning. Results add to a half-dozen already known RC Li-rich K giants and support the growing evidence that the origin of Li excess in RC giants seems to be associated with either He flash at the tip of the RGB or recent planet/ brown dwarf merger events closer to the RGB tip.