An analysis of the abundances of the Silicon star HD 206653 is presented using an ATLAS9 model atmosphere and observational material taken with a REOSC echelle spectrograph attached to the Jorge Sahade 2.15 m telescope at CASLEO. The light elements are solar or deficient except silicon which is overabundant by a factor of 5. The iron peak elements are all overabundant by factors between 10 and 50. Sr and Y are around 1000 times the solar values. Among the Rare Earths only Ce and Eu are identified; both are overabundant by large factors
We report on VLT/UVES high-resolution spectra of four members of the old metal-rich open cluster NGC...
Context. Moderately r-process-enriched stars (r-I; +0.3 ≤ [Eu/Fe] ≤ +1.0) are at least four times...
Spectra obtained with the ESO Cassegrain echelle spectrograph are used to determine the abundances o...
An analysis of the abundances of the Silicon star HD 206653 is presented using an ATLAS9 model atmos...
Fine analyses of the silicon stars HD 133029 and HD 192913 are presented using ATLAS9 model atmosphe...
Abundance analysis using optical region data and fully line blanketed model atmospheres have been pe...
An elemental abundance analysis of the cool magnetic CP star HR 8216 (= HD204411) was performed usin...
Atmospheric parameters and chemical abundances of HD 161480 were determined by means of spectrograms...
International audienceAims. In order to provide a better basis for the study of mechanisms of nucleo...
The elemental composition of the chemically peculiar star HR 6958 has been studied with emphasis on ...
High resolution spectrophotometric data were obtained for the stellar objects HD 19445 and HD 140283...
We examine the sharp-lined stars HR 6455 (A3 III, v sin i = 8.7 km s -1) and \u3b7 Lep (F2 V, v sin ...
Context. The sharp-line spectrum of the non-magnetic, main-sequence Bp star HR 6000 has peculiaritie...
International audienceWe test the capabilities of 0.4 m telescopes equipped with an échelle spectrog...
In this paper we present an analysis of the Ap(Si) stars HD 87405 and HD 146555 using an ATLAS9 mode...
We report on VLT/UVES high-resolution spectra of four members of the old metal-rich open cluster NGC...
Context. Moderately r-process-enriched stars (r-I; +0.3 ≤ [Eu/Fe] ≤ +1.0) are at least four times...
Spectra obtained with the ESO Cassegrain echelle spectrograph are used to determine the abundances o...
An analysis of the abundances of the Silicon star HD 206653 is presented using an ATLAS9 model atmos...
Fine analyses of the silicon stars HD 133029 and HD 192913 are presented using ATLAS9 model atmosphe...
Abundance analysis using optical region data and fully line blanketed model atmospheres have been pe...
An elemental abundance analysis of the cool magnetic CP star HR 8216 (= HD204411) was performed usin...
Atmospheric parameters and chemical abundances of HD 161480 were determined by means of spectrograms...
International audienceAims. In order to provide a better basis for the study of mechanisms of nucleo...
The elemental composition of the chemically peculiar star HR 6958 has been studied with emphasis on ...
High resolution spectrophotometric data were obtained for the stellar objects HD 19445 and HD 140283...
We examine the sharp-lined stars HR 6455 (A3 III, v sin i = 8.7 km s -1) and \u3b7 Lep (F2 V, v sin ...
Context. The sharp-line spectrum of the non-magnetic, main-sequence Bp star HR 6000 has peculiaritie...
International audienceWe test the capabilities of 0.4 m telescopes equipped with an échelle spectrog...
In this paper we present an analysis of the Ap(Si) stars HD 87405 and HD 146555 using an ATLAS9 mode...
We report on VLT/UVES high-resolution spectra of four members of the old metal-rich open cluster NGC...
Context. Moderately r-process-enriched stars (r-I; +0.3 ≤ [Eu/Fe] ≤ +1.0) are at least four times...
Spectra obtained with the ESO Cassegrain echelle spectrograph are used to determine the abundances o...