Published in

Oxford University Press, Publications of Astronomical Society of Japan, 2(53), p. 315-320, 2001

DOI: 10.1093/pasj/53.2.315

Links

Tools

Export citation

Search in Google Scholar

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

Journal article published in 2001 by Kozo Sadakane, Michiko Ohkubo, Shizuka Sato, Kyoichi Osada, Masahide Takada-Hidai, Seiji Masuda, Hideyuki Izumiura, Hisashi Koyano, Fumihiro Uraguchi, Hideo Maehara, Etsuji Watanabe, Yuji Norimoto, Kenshi Yanagisawa ORCID, Takafumi Okada, Yasuhiro Shimizu and other authors.
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Upload
Orange circle
Postprint: archiving restricted
Upload
Red circle
Published version: archiving forbidden
Policy details
Data provided by SHERPA/RoMEO

Abstract

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 Teff = 5500 +/- 100 K,log g = 3.6 +/- 0.1, xit = 1.0 +/- 0.3 km s-1, and [M/H] = +0.3. Iron is definitely overabundant with respect to the Sun, [Fe/H] = +0.40 +/- 0.06, and all other elements are also found to be enhanced. The enhancements of iron peak elements (Ti through Ni) are coincident with that of Fe within +/- 0.1 dex, while C and O are slightly less enhanced than Fe.