-
Chemical composition of the s-Cepheids
On the base of photographic, Reticon and CCD spectra analysis we have derived the abundances for 8 s-Cepheids and V1162 Aql (before classified as s-Cepheid). The following... -
Fe I in metal-poor stars
A detailed analysis of neutral iron lines in a sample of 13 metal-poor dwarfs and subgiants is carried out on the basis of high resolution spectra obtained with the ESO Coude... -
Abundances in zeta Scl open cluster
(no description available) -
LMC F supergiants
(no description available) -
Abundances of very metal-poor stars
(no description available) -
Galactic abundance gradients
(no description available) -
Catalogue of [Fe/H] of F, G, K stars
The catalogue presented here is a compilation of published atmospheric parameters (Teff, logg, [Fe/H]) obtained from high resolution, high signal-to-noise spectroscopic... -
Catalogue of [Fe/H]
The catalogue includes [Fe/H] determinations and atmospheric parameters (Teff, logg ) obtained from high resolution spectroscopic observations and detailed analyses, most of... -
Chemical Abundances in Late-Type Stars
The catalogue includes chemical abundances determinations (from Li to Eu) and atmospheric parameters (Teff, logg, microturbulent velocity) obtained from re-analyses of 1108... -
The PASTEL catalogue
PASTEL is a bibliographical catalogue compiling determinations of stellar atmospheric parameters. It provides (Teff, logg, [Fe/H]) determinations obtained from detailed analyses... -
Atmospheric parameters in metal-poor stars. I
We present atmospheric parameters for about 300 stars of different chemical composition, whose spectra will be used to study the galactic enrichment of Fe and light elements.... -
Abundances for lines of n-capture in 19 stars
(no description available) -
Molecules in O- and C-rich envelopes
Observations of 10 microwave transitions of the molecules SiO, HCN, HNC, SiS, HC_3_N, CS, SO, and ^13^CO are presented in a total sample of 47 evolved stars. The studied sources... -
Abundances in NGC 2243 and Mel 66
(no description available) -
Abundance gradients from disk PNs
A new determination of the radial abundance gradients of O/H, Ne/H, S/H, and Ar/H is made for disk planetary nebulae, (PN), that is, those objects of Peimbert types I, II, and... -
Chemical abundances of PNe
All modern determinations of chemical abundances of He/H, O/H, C/H, N/H and Ne/H in 277 galactic Planetary Nebulae have been used to update our knowledge of the chemical... -
Abundances of non-type I PNe in LMC
Spectroscopic observations, plasma diagnostics and chemical composition of 15 non-type I planetary nebulae (PNe) in the Large Magellanic Cloud (LMC) are reported. Abundances of... -
Chemical evolution of the galactic disk I.
From high resolution, high S/N spectroscopic observations of carefully selected northern and southern stars, abundances of O, Na, Mg, Al, Si, Ca, Ti, Fe, Ni, Y, Zr, Ba and Nd,... -
APOGEE-2 DR17 final allStar catalog
The 2022ApJS..259...35A paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17... -
Abundances of late G/K dwarfs in solar neighborhood
In this investigation, a technique developed by Spinrad and Taylor for obtaining metal abundances of late-type stars, and used by them in an earlier investigation of evolved...
