Equivalent widths of 3 post-AGB Virtual Observatory Resource

Authors

1. Mooney C.J.
2. Rolleston W.R.J.
3. Keenan F.P.
4. Dufton P.L.
5. Smoker J.V.,Ryans R.S.I.
6. Aller L.H.
7. Trundle C.

Published by

CDS

Abstract

We present model atmosphere analyses of high resolution Keck and VLT optical spectra for three evolved stars in globular clusters, viz. ZNG-1 in M10, ZNG-1 in M15 and ZNG-1 in NGC6712. The derived atmospheric parameters and chemical compositions confirm the programme stars to be in the post-Asymptotic Giant Branch (post-AGB) evolutionary phase.

Keywords

1. globular-star-clusters
2. early-type-stars
3. line-intensities

Bibliographic source Bibcode

2004A&A...419.1123M

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/419/1123

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/419/1123

Document Object Identifer DOI

doi:10.26093/cds/vizier.34191123

Access

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http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/419/1123
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http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/419/1123

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