Add to ORKGA synthetic spectrum analysis of CCD observations in the spectral region λλ 6400-6500 ÅÅ of the stars HD 155375, HD 159560, and HD 196544 was carried out. All stars show typical Am characteristics
We present new orbits for sixteen Ap spectroscopic binaries, four of which might in fact be Am stars...
The combination of photometry, spectroscopy and spectropolarimetry of the chemically peculiar stars ...
The new spectropolarimetric spectra of HD 157087 obtained recently with ESPaDOnS at CFHT are analyse...
We continue here the systematic abundance analysis of a sample of Am binaries in order to search for...
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...
We aim to carry out a study on the photometric and spectroscopic variabilities of four stars monitor...
An abundance analysis using photographic region spectrograms and fully line-blanketed model atmosphe...
Context. Modern spectroscopy of early-type stars often aims at studying complex physical phenomena ...
We used high-resolution echelle spectra acquired with the 1. 5-m Russian-Turkish Telescope to determ...
International audienceWe report on a detailed abundance study of six bright, mostly southern, slowly...
NOTE: Text or symbols not renderable in Plain ACII are indicated by [...]. Abstract is included in ....
Context.The γ Doradus stars are a recent class of variable main sequence F-type stars located on the...
We have analysed the chemical photospheric composition of 24 Herbig Ae/Be and Vega-type stars in se...
Context. The current knowledge of the abundance pattern in δ Scuti stars is based on analysis of jus...
We present new orbits for sixteen Ap spectroscopic binaries, four of which might in fact be Am stars...
The combination of photometry, spectroscopy and spectropolarimetry of the chemically peculiar stars ...
The new spectropolarimetric spectra of HD 157087 obtained recently with ESPaDOnS at CFHT are analyse...
We continue here the systematic abundance analysis of a sample of Am binaries in order to search for...
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...
We aim to carry out a study on the photometric and spectroscopic variabilities of four stars monitor...
An abundance analysis using photographic region spectrograms and fully line-blanketed model atmosphe...
Context. Modern spectroscopy of early-type stars often aims at studying complex physical phenomena ...
We used high-resolution echelle spectra acquired with the 1. 5-m Russian-Turkish Telescope to determ...
International audienceWe report on a detailed abundance study of six bright, mostly southern, slowly...
NOTE: Text or symbols not renderable in Plain ACII are indicated by [...]. Abstract is included in ....
Context.The γ Doradus stars are a recent class of variable main sequence F-type stars located on the...
We have analysed the chemical photospheric composition of 24 Herbig Ae/Be and Vega-type stars in se...
Context. The current knowledge of the abundance pattern in δ Scuti stars is based on analysis of jus...
We present new orbits for sixteen Ap spectroscopic binaries, four of which might in fact be Am stars...
The combination of photometry, spectroscopy and spectropolarimetry of the chemically peculiar stars ...
The new spectropolarimetric spectra of HD 157087 obtained recently with ESPaDOnS at CFHT are analyse...