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Non-LTE Line-Formation and Abundances of Sulfur and Zinc in F, G, and K Stars
- Y. Takeda, O. Hashimoto, S. Honda
- Physics
- 9 September 2005
Extensive statistical-equilibrium calculations on neutral sulfur and zinc were carried out, in order to investigate how the non-LTE effect plays a role in the determination of S and Zn abundances in…
Oxygen line formation in late-F through early-K disk/halo stars. Infrared O I triplet and [O I] lines
- Y. Takeda
- Physics
- 14 May 2001
In order to investigate the formation of O 7771-5 and (O ) 6300/6363 lines, extensive non-LTE calculations for neutral atomic oxygen were carried out for wide ranges of model atmosphere…
Stellar Parameters and Elemental Abundances of Late-G Giants
The properties of 322 intermediate-mass late-G giants (comprising 10 planet-host stars) selected as the targets of the Okayama Planet Search Program, many of which are red-clump giants, were…
Photospheric CNO Abundances of Solar-Type Stars
We determined the C, N, and O abundances of 160 nearby F, G, and K dwarfs and subgiants by using spectra obtained with the HIDES spectrograph at Okayama Astrophysical Observatory, with the purposes…
Planetary Companions around Three Intermediate-Mass G and K Giants: 18 Delphini, ξ Aquilae, and HD 81688
- B. Sato, H. Izumiura, S. Ida
- Physics, Geology
- 19 February 2008
We report on the detection of 3 new extrasolar planets from a precise Doppler survey of G and K giants at Okayama Astrophysical Observatory. The host stars, 18 Del (G6 III), � Aql (K0 III) and HD…
Fundamental Parameters and Elemental Abundances of 160 F-G-K Stars Based on OAO Spectrum Database
- Y. Takeda
- Physics
- 25 April 2007
The properties of 160 F, G, and K disk dwarfs/subgiants (including 27 planet-host stars) mostly within � 0:6 . [Fe/H] . +0:4 ,t he Okayama Astrophysical Observatory spectrum collection of which had…
Non-LTE Analysis of the Sodium Abundance of Metal-Poor Stars in the Galactic Disk and Halo
- Y. Takeda, Gang Zhao, M. Takada-Hidai, Yuqin Chen, Yu-ji Saito, Huawei Zhang
- Physics
- 18 April 2003
We performed an extensive non-LTE analysis of the neutral sodium lines of Na i 5683/5688, 5890/5896, 6154/6161, and 8183/8195 in disk/halo stars of types F-K covering a wide metallicity range ( 4 <…
A Planetary Companion to the Hyades Giant ∊ Tauri
- B. Sato, H. Izumiura, S. Ida
- Physics, Geology
- 20 May 2007
Wereportthedetection of anextrasolarplanet orbitingTau,oneof thegiantstarsintheHyadesopencluster.This is the first planet ever discovered in an open cluster. Precise Doppler measurements of this star…
Spectroscopic Study on the Atmospheric Parameters of Nearby F-K Dwarfs and Subgiants
- Y. Takeda, M. Ohkubo, B. Sato, E. Kambe, K. Sadakane
- Physics
- 25 February 2005
Based on a collection of high-dispersion spectra obtained at Okayama Astrophysical Observatory, the atmospheric parameters (Teff ,l ogg, vt ,a nd [Fe/H]) of 160 mid-F through early-K stars were…
Lithium Abundances of F-, G-, and K-Type Stars: Profile-Fitting Analysis of the Li I 6708 Doublet
- Y. Takeda, S. Kawanomoto
- Physics, Geology
- 25 February 2005
An extensive profile-fitting analysis was performed for the Li(+Fe) 6707–6708 u A feature of nearby 160 F–K dwarfs/subgiants (including 27 planet-host stars) in the Galactic disk (7000K Teff5000K,…
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