[Be] abundances in low-metallicity stars (Molaro+ 1997)

Details [Be] abundances in low-metallicity stars (Molaro+ 1997) [Be] abundances in low-metallicity stars (Molaro+ 1997)

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..33190593m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/319/593. Originally published in: 1997A&A...319..593M

Physics

Stars: Metal-Deficient, Abundances

Scientific paper

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 spectrograph of the ESO 3.6m telescope at a FWHM=~8.6km/s resolution. Abundances are derived by means of the synthetic spectra technique employing Kurucz (1993, CD-ROM 13 and CD-ROM 18) atmospheric models, with enhanced α-elements and no overshooting. (4 data files).

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