2015A&A...581A..94A


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.03CEST23:06:06

2015A&A...581A..94A - Astronomy and Astrophysics, volume 581A, 94-94 (2015/9-1)

Tracking Advanced Planetary Systems (TAPAS) with HARPS-N. II. Super Li-rich giant HD 107028.

ADAMOW M., NIEDZIELSKI A., VILLAVER E., WOLSZCZAN A., KOWALIK K., NOWAK G., ADAMCZYK M. and DEKA-SZYMANKIEWICZ B.

Abstract (from CDS):

Lithium-rich giant stars are rare objects. For some of them, Li enrichment exceeds the abundance of this element found in solar system meteorites, suggesting that these stars have gone through a Li enhancement process. We identified a Li-rich giant HD 107028 with A(Li)>3.3 in a sample of evolved stars observed within the PennState Torun Planet Search. In this work we study different enhancement scenarios and we try to identify the one responsible for Li enrichment in HD 107028. We collected high-resolution spectra with three different instruments, covering different spectral ranges. We determined stellar parameters and abundances of selected elements with both equivalent width measurements and analysis, and spectral synthesis. We also collected multi-epoch high-precision radial velocities in an attempt to detect a companion. Collected data show that HD 107028 is a star at the base of the red giant branch (RGB). Except for high Li abundance, we have not identified any other anomalies in its chemical composition, and there is no indication of a low-mass or stellar companion. We exclude Li production at the luminosity function bump on the RGB as the effective temperature and luminosity suggest that the evolutionary state is much earlier than the RGB bump. We also cannot confirm the Li enhancement by contamination as we do not observe any anomalies that are associated with this scenario. After evaluating various scenarios of Li enhancement we conclude that the Li-overabundance of HD 107028 originates from main-sequence evolution, and may be caused by diffusion processes.

Abstract Copyright:

Journal keyword(s): stars: individual: HD 107028 - stars: late-type - stars: fundamental parameters - stars: atmospheres - techniques: spectroscopic - planetary systems

Simbad objects: 6

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Number of rows : 6

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 BD+48 740 * 02 42 58.2182761768 +48 55 48.225888943   10.05 8.70     K3III 26 0
2 SDSS J072042.79+303651.4 HB? 07 20 42.7899174202 +30 36 51.503809456           ~ 4 0
3 HD 107028 PM* 12 18 00.2430777360 +68 47 49.348622636   8.47 7.64 11.8   G5 14 1
4 NGC 6397 GlC 17 40 42.09 -53 40 27.6   7.39 5.17     ~ 1798 1
5 NGC 6633 47 * 18 26 32.2713970101 +06 23 08.953014385   11.39 10.92     A9 22 0
6 NGC 6633 OpC 18 27 31.2 +06 34 12           ~ 323 0

    Equat.    Gal    SGal    Ecl

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2020.07.03-23:06:06

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