Elemental abundances for HgMn stars observed with EBASIM echelle spectrograph at CASLEO

Details Elemental abundances for HgMn stars observed with EBASIM echelle spectrograph at CASLEO Elemental abundances for HgMn stars observed with EBASIM echelle spectrograph at CASLEO

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..224..662p&link_type=abstract

The A-Star Puzzle, held in Poprad, Slovakia, July 8-13, 2004. Edited by J. Zverko, J. Ziznovsky, S.J. Adelman, and W.W. Weiss,

Astronomy and Astrophysics

Astrophysics

Stars: Abundances, Individual:(Hr 4817, Μ Lep), Stars: Chemically Peculiar Stars.

Scientific paper

Elemental abundance analysis are derived for the Mercury-Manganese stars HR 4817 (B8 II/III) and μ Lep (B9 IV) using CCD recorded exposures obtained at the EBASIM echelle spectrograph at the 2.1-m CASLEO (Complejo Astronómico El Leoncito) telescope in Argentina. The spectra coverage is 390-900 nm. The results are compared with previous analyses made with spectra taken using the REOSC echelle spectrograph at CASLEO, the coudé feed telescope at Kitt Peak National Observatory, and/or with the Dominion Astrophysical Observatory coudé spectrograph. As these new spectra go farther into the red and have better resolution than those obtained with the REOSC, we could make better abundance determinations.

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