Planetary nebulae with WR-type nuclei Virtual Observatory Resource

Authors
  1. GORNY S.K.
  2. STASINSKA G.
  3. Published by
    CDS
Abstract

A recent systematic search of Wolf-Rayet features in the spectra of Galactic planetary nebulae has increased the list of objects that are known to have WR-type nuclei to about 50. We have compared their nebular properties with those of the other planetary nebulae in the Galaxy.

Keywords
  1. wolf-rayet-stars
Bibliographic source Bibcode
1995A&A...303..893G
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/303/893
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/303/893
Document Object Identifer DOI
doi:10.26093/cds/vizier.33030893

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/303/893
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/303/893
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/303/893
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

1997-12-09T17:36:41Z
Resource record created
1997-12-09T16:36:45Z
Updated
1997-12-09T17:36:41Z
Created

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