Galactic PNe abundances Virtual Observatory Resource

Authors

1. Perinotto M.
2. Morbidelli L.
3. Scatarzi A.

Published by

CDS

Abstract

New determinations of chemical abundances for He, N, O, Ne, Ar and S are derived for all galactic planetary nebulae (PNe) so far observed with a relatively high accuracy, in an effort to overcome differences in these quantities obtained over the years by different authors using different procedures.

Keywords

1. planetary-nebulae
2. chemical-abundances

Bibliographic source Bibcode

2004MNRAS.349..793P

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/349/793

IVOA Identifier IVOID

ivo://CDS.VizieR/J/MNRAS/349/793

Document Object Identifer DOI

doi:10.26093/cds/vizier.73490793

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/349/793
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/349/793
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/349/793

IVOA Table Access TAP

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

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/349/793/sample?
https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/349/793/sample?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/349/793/sample?