Galactic PNe abundances

DOI

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.

Cone search capability for table J/MNRAS/349/793/sample (Planeraty nebulae positions (from Simbad))

Identifier
DOI http://doi.org/10.26093/cds/vizier.73490793
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/349/793
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/349/793
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/349/793
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/349/793
Provenance
Creator Perinotto M.; Morbidelli L.; Scatarzi A.
Publisher CDS
Publication Year 2007
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Interstellar medium; Natural Sciences; Physics