144 citations · 217 across the 3 of their papers we have counts for
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Reddenings of FGK supergiants and classical Cepheids from spectroscopic data
V. V. Kovtyukh, C. Soubiran, R. E. Luck +4
Accurate and homogeneous atmospheric parameters (Teff, log (g), Vt, [Fe/H]) are derived for 74 FGK non-variable supergiants from high-resolution, high signal-to-noise ratio, echell…
Elemental abundances in the atmosphere of clump giants
T. V. Mishenina, O. Bienaym'e, T. I. Gorbaneva +4
The aim of this paper is to provide the fundamental parameters and abundances for a large sample of local clump giants with a high accuracy. The selection of clump stars for the sa…
Vertical distribution of Galactic disk stars: III. The Galactic disk surface mass density from red clump giants
O. Bienaymé, C. Soubiran, T. V. Mishenina +2
We used red clump stars to measure the surface mass density of the Galactic disk in the solar neighbourhood. High resolution spectra of red clump stars towards the NGP have been ob…
A new Bohm-Vitense gap in the temperature range 5560 to 5610K in the Main Sequence
V. V. Kovtyukh, C. Soubiran, S. I. Belik
Highly precise temperatures (sigma = 10-15 K) have been determined from line depth ratios for a set of 248 F-K field dwarfs of about solar metallicity (-0.5 < [Fe/H] < +0.4), based…
On the correlation of elemental abundances with kinematics among galactic disk stars
T. V. Mishenina, C. Soubiran, V. V. Kovtyukh +1
We have performed the detailed analysis of 174 high-resolution spectra of FGK dwarfs obtained with the ELODIE echelle spectrograph at the Observatoire de Haute-Provence. Abundances…
High precision effective temperatures for 181 F--K dwarfs from line-depth ratios
V. V. Kovtyukh, C. Soubiran, S. I. Belik +1
Line depth ratios measured on high resolution (R=42000), high S/N echelle spectra are used for the determination of precise effective temperatures of 181 F,G,K Main Sequence stars…