THE PAN-PACIFIC PLANET SEARCH. V. FUNDAMENTAL PARAMETERS FOR 164 EVOLVED STARS

被引:15
|
作者
Wittenmyer, Robert A. [1 ,2 ,3 ]
Liu, Fan [4 ]
Wang, Liang [5 ,6 ]
Casagrande, Luca [4 ]
Johnson, John Asher [7 ]
Tinney, C. G. [1 ,2 ]
机构
[1] UNSW Australia, Sch Phys, Sydney, NSW 2052, Australia
[2] UNSW Australia, Australian Ctr Astrobiol, Sydney, NSW 2052, Australia
[3] Univ Southern Queensland, Computat Engn & Sci Res Ctr, Toowoomba, Qld 4350, Australia
[4] Australian Natl Univ, Res Sch Astron & Astrophys, Cotter Rd, Weston, ACT 2611, Australia
[5] Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, A20 Datun Rd, Beijing 100012, Peoples R China
[6] Max Planck Inst Extraterr Phys, Giessenbachstr, D-85748 Garching, Germany
[7] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
来源
ASTRONOMICAL JOURNAL | 2016年 / 152卷 / 01期
关键词
stars: fundamental parameters; techniques: spectroscopic; RELATIVE OSCILLATOR-STRENGTHS; PRECISE RADIAL-VELOCITIES; FE-I TRANSITIONS; GIANT STARS; CHEMICAL-COMPOSITION; STELLAR PARAMETERS; MAIN-SEQUENCE; METALLICITY; MASS; ABUNDANCES;
D O I
10.3847/0004-6256/152/1/19
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present spectroscopic stellar parameters for the complete target list of 164 evolved stars from the Pan-Pacific Planet Search, a five-year radial velocity campaign using the 3.9 m Anglo-Australian Telescope. For 87 of these bright giants, our work represents the first determination of their fundamental parameters. Our results carry typical uncertainties of 100 K, 0.15 dex, and 0.1 dex in T-eff, log g, and [Fe/H] and are consistent with literature values where available. The derived stellar masses have a mean of 1.31(-0.25)(+0.28) M-circle dot, with a tail extending to similar to 2 M-circle dot, consistent with the interpretation of these targets as "retired" A-F type stars.
引用
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页数:15
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