Interacting planetary nebulae

DOI

We discuss the classification and orientation of planetary nebulae that interact with the interstellar medium throughout the Milky Way. A sample of 117 confirmed interacting planetary nebulae is used for this purpose. Our results indicate that the majority of interacting objects are located close to the Galactic plane, and ~77% of them are located inside the Galactic thin disk.

Cone search capability for table J/A+A/541/A98/table1 (The main parameters of the interacting planetary nebulae sample)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35410098
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/541/A98
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/541/A98
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/541/A98
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/541/A98
Provenance
Creator Ali A.; Sabin L.; Snaid S.; Basurah H.M.
Publisher CDS
Publication Year 2012
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