Chemical abundances of planetary nebulae

DOI

In this paper, we report new observations and derive chemical abundances for a sample of 26 planetary nebulae (PN) located in the anti-center direction. Most of these nebulae are far away objects, located at galactocentric distances greater than about 8kpc, so that they are particularly useful for the determination of the radial gradients at large distances from the galactic center.

Cone search capability for table J/A+A/423/199/table1 (Log of the observations and distances)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34230199
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/423/199
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/423/199
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/423/199
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/423/199
Provenance
Creator Costa R.D.D.; Uchida M.M.M.; Maciel W.J.
Publisher CDS
Publication Year 2004
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; Interstellar medium; Natural Sciences; Physics; Stellar Astronomy