Elemental abundance analyses IV. Virtual Observatory Resource

Authors

1. Adelman S.J.
2. Pintado O.I.

Published by

CDS

Abstract

Using new CASLEO echelle spectrograms, we extended our elemental abundances of the sharp-lines Mercury-Manganese star {mu} Lep, 14 Hya, {kappa} Cnc, HR 4487, 28 Her, and HR 7245, the closely related star 3 CenA, and 7 Sex an A0V star with population I abundances, but with Population II star space motion. The {lambda}{lambda}4500-6200 region contains a sufficient number of lines to derive high-quality abundances of these stars. For most stars, the new spectra provide additional lines for the analyses which improve their quality as well as help fill in the periodic table.

Keywords

1. peculiar-variable-stars
2. chemically-peculiar-stars

Bibliographic source Bibcode

2000A&A...354..899A

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/354/899

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/354/899

Document Object Identifer DOI

doi:10.26093/cds/vizier.33540899

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/354/899
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/354/899
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/354/899

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).