333 datasets found

Keywords: chemically peculiar stars

Filter Results
  • Chemical abundances of planetary nebulae

    In this paper, we report new observations and derive chemical abundances for a sample of 26 planetary nebulae (PN) located in the anti-center direction. Most of these nebulae...
  • Metal-poor star uvby-beta photometry. X.

    (uvby) and H-beta photometry has been obtained for an additional 411 very metal-poor stars selected from the HK survey, and used to derive basic parameters such as interstellar...
  • Abundances in the Sgr dSph

    We report on abundances of O, Mg, Si, Ca and Fe for 10 giants in the Sgr dwarf spheroidal derived from high resolution spectra obtained with UVES at the 8.2m Kueyen-VLT...
  • Li abundances and velocities in F and G stars

    Lithium abundances have been determined in 127 F and G Pop I stars based on new measurements of the equivalent width of the {lambda}6707{AA} Li I line from their high resolution...
  • IR O I triplet, [O I] lines in F-K dwarfs/giants

    In order to investigate the formation of O I 7771-5 and [O I] 6300/6363 lines, extensive non-LTE calculations for neutral atomic oxygen were carried out for wide ranges of model...
  • Statistical properties of exoplanets II

    Table2 file is an extended version of table 2 in the paper. It contains the stellar parameters as well as the number of FeI and FeII lines used (and the rms around the mean...
  • Chemical compositions of four barium stars

    Chemical compositions of four barium stars are studied. We obtain their {alpha}, iron peak and neutron-capture (n-capture) process element abundances. The atomic data and...
  • Abundances of PN towards Galactic bulge

    In this work we report spectrophotometric observations of a planetary nebula sample towards the galactic bulge. A total of 45 PNe was observed and their physical parameters...
  • Elemental abundance of 4 normal B and A stars

    Elemental abundances analysis of the superficially normal B and A stars {alpha} Dra (A0 III), {tau} Her (B5 IV), {gamma} Lyr (B9 III), and HR 7926 (B8 II-III) are performed...
  • {alpha} Scl and HD 170973 abundances

    Fine analyses of the magnetic CP stars {alpha} Scl and HD 170973 are presented using ATLAS9 model atmospheres which have same bulk metallicity as the deduced abundances. The...
  • ups Her, phi Her & HR 7018 abundances

    Elemental abundances analyses are performed for the Mercury-Manganese stars {upsilon} Her, {phi} Her, and HR 7018 consistent with previous studies of this series using...
  • Elemental abundances of Deneb

    This study presents a detailed model atmosphere abundance analysis of Deneb which was performed using Kurucz LTE ATLAS9 model atmospheres. The atmospheric parameters were...
  • Atmospheric parameters in metal-poor stars. II

    We present non-LTE corrections to abundances of Fe, O, Na, and Mg derived from LTE analyses of F-K stars over a broad range of gravities and metal abundances; they were obtained...
  • Abundance gradients in planetary nebulae

    Radial abundance gradients of the element ratios O/H, Ne/H, S/H, and Ar/H are determined on the basis of a sample of disk planetary nebulae. The behaviour of the gradients at...
  • The red spectrum of HD 101065

    Wavelength list for Przybylski's star (a rapidly rotation Ap star) including a measurement of the line depths.
  • Abundances of 9 solar-type stars

    Line identifications, measured equivalent widths and derived chemical abundances in 9 solar-type dwarf stars, which are identified by their Bright Star (HR, (Cat. )) numbers.
  • [Be] abundances in low-metallicity stars

    We present observations of the Be II 313.0nm resonance doublet in 14 halo and old disk stars with metallicities ranging from [Fe/H]=-0.4 to =~-3.0 obtained with the CASPEC...
  • 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....
  • Metal-poor stars spectroscopy. II

    Models of post-main sequence stellar evolution of VandenBerg & Bell have been applied to determine spectroscopic masses and distances for metal-poor stars. Careful...
  • Abundances of very metal-poor stars

    (no description available)
You can also access this registry using the API (see API Docs).