Equivalent widths of two post-AGB stars Virtual Observatory Resource

Authors
  1. Reyniers M.
  2. Van Winckel H.
  3. Gallino R.
  4. Straniero O.
  5. Published by
    CDS
Abstract

In an effort to extend the still limited sample of s-process enriched post-AGB stars, high-resolution, high signal-to-noise VLT+UVES spectra of the optical counterparts of the infrared sources IRAS 06530-0213 and IRAS 08143-4406 were analysed.

Keywords
  1. infrared-sources
  2. line-intensities
  3. chemical-abundances
  4. spectroscopy
Bibliographic source Bibcode
2004A&A...417..269R
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/417/269
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/417/269
Document Object Identifer DOI
doi:10.26093/cds/vizier.34170269

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/417/269
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/417/269
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/417/269
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2004-06-05T21:01:21Z
Resource record created
2004-06-05T21:01:21Z
Created
2004-06-05T21:01:25Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr