An abundance analysis using photographic region spectrograms and fully line-blanketed model atmospheres has been performed for the chemically peculiar (CP) star HD 26385. Model parameters were determined from H-gamma-profile and photometric data. Its pattern of abundance shows that HD 26385 is typically Ap Si-star
Context. The current knowledge of the abundance pattern in δ Scuti stars is based on analysis of jus...
The new spectropolarimetric spectra of HD 157087 obtained recently with ESPaDOnS at CFHT are analyse...
We have performed abundance analysis of two slowly rotating, late A-type stars, HD 32115 (HR 1613) ...
Atmospheric parameters and chemical abundances of HD 161480 were determined by means of spectrograms...
NOTE: Text or symbols not renderable in Plain ACII are indicated by [...]. Abstract is included in ....
A synthetic spectrum analysis of CCD observations in the spectral region λλ 6400-6500 ÅÅ of the star...
Aims. Among the known Ap stars, HD 101065 is probably one of the most interesting objects, demonstra...
Context.High spectral resolution studies of cool Ap stars reveal conspicuous anomalies of the shape ...
Context. Chemically peculiar (CP) stars are unique natural laboratories for the investigation of the...
Context: High-resolution spectra of some chemically peculiar stars clearly demonstrate the presence ...
Abundance analysis using optical region data and fully line blanketed model atmospheres have been pe...
An analysis of the abundances of the Silicon star HD 206653 is presented using an ATLAS9 model atmo...
We present the results of our determination of the fundamental atmospheric parameters for the magnet...
Fine analyses of the silicon stars HD 133029 and HD 192913 are presented using ATLAS9 model atmosphe...
We have identified the atomic species present in the spectrum of the CP star HR 8137 (HD 202671 = 30...
Context. The current knowledge of the abundance pattern in δ Scuti stars is based on analysis of jus...
The new spectropolarimetric spectra of HD 157087 obtained recently with ESPaDOnS at CFHT are analyse...
We have performed abundance analysis of two slowly rotating, late A-type stars, HD 32115 (HR 1613) ...
Atmospheric parameters and chemical abundances of HD 161480 were determined by means of spectrograms...
NOTE: Text or symbols not renderable in Plain ACII are indicated by [...]. Abstract is included in ....
A synthetic spectrum analysis of CCD observations in the spectral region λλ 6400-6500 ÅÅ of the star...
Aims. Among the known Ap stars, HD 101065 is probably one of the most interesting objects, demonstra...
Context.High spectral resolution studies of cool Ap stars reveal conspicuous anomalies of the shape ...
Context. Chemically peculiar (CP) stars are unique natural laboratories for the investigation of the...
Context: High-resolution spectra of some chemically peculiar stars clearly demonstrate the presence ...
Abundance analysis using optical region data and fully line blanketed model atmospheres have been pe...
An analysis of the abundances of the Silicon star HD 206653 is presented using an ATLAS9 model atmo...
We present the results of our determination of the fundamental atmospheric parameters for the magnet...
Fine analyses of the silicon stars HD 133029 and HD 192913 are presented using ATLAS9 model atmosphe...
We have identified the atomic species present in the spectrum of the CP star HR 8137 (HD 202671 = 30...
Context. The current knowledge of the abundance pattern in δ Scuti stars is based on analysis of jus...
The new spectropolarimetric spectra of HD 157087 obtained recently with ESPaDOnS at CFHT are analyse...
We have performed abundance analysis of two slowly rotating, late A-type stars, HD 32115 (HR 1613) ...
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