Metallic Abundances in the Planet-Harboring G-Type Star HD 38529 | Zendy

Kozo Sadakane | Zendy; Michiko Ohkubo | Zendy; S. Sato | Zendy; Kyoichi Osada | Zendy; Masahide TakadaHidai | Zendy; Seiji Masuda | Zendy; Hideyuki Izumiura | Zendy; Hisashi Koyano | Zendy; H. Maehara | Zendy; Yuji Norimoto | Zendy; Takafumi Okada | Zendy; Yasuhiro Shimizu | Zendy; Fumihiro Uraguchi | Zendy; E. Watanabe | Zendy; K. Yanagisawa | Zendy; M. Yoshida | Zendy

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Metallic Abundances in the Planet-Harboring G-Type Star HD 38529

Author(s) -

Kozo Sadakane,

Michiko Ohkubo,

S. Sato,

Kyoichi Osada,

Masahide TakadaHidai,

Seiji Masuda,

Hideyuki Izumiura,

Hisashi Koyano,

H. Maehara,

Yuji Norimoto,

Takafumi Okada,

Yasuhiro Shimizu,

Fumihiro Uraguchi,

E. Watanabe,

K. Yanagisawa,

M. Yoshida

Publication year - 2001

Publication title -

publications of the astronomical society of japan

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.99

H-Index - 110

eISSN - 2053-051X

pISSN - 0004-6264

DOI - 10.1093/pasj/53.2.315

Subject(s) - physics , planet , star (game theory) , astrophysics , metal , analytical chemistry (journal) , environmental chemistry , chemistry , organic chemistry

The abundances of 16 elements (C through Y) in the recently detected planet-harboring G4 IV star HD 38529 are presented. A spectroscopic analysis was carried out differentially relative to the Sun. The adopted atmospheric parameters of the star are $T_{\rm eff} = 5500 \pm 100 ~ {\rm K}, \log g = 3.6 \pm 0.1, \xi_{\rm t}= 1.0 \pm 0.3 ~ {\rm km} ~ {\rm s}^{-1}$, and [M/H]$= +0.3$. Iron is definitely...

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