M 2-9 ^12^CO and ^13^CO channel maps

DOI

M 2-9 is a young planetary nebula (PN) that shows the characteristics of its last ejections in unprecedented detail. These last ejections are thought to trigger the post-asymptotic giant branch evolution. To assemble an overall picture of how M 2-9 was shaped, we analyzed the characteristics of the different molecular gas components and their relation with the warmer parts of the nebula that are visible in the optical domain. ^12^CO and ^13^CO J=3-2 line emission maps were obtained with the Atacama Large Millimeter/submillimeter Array with high angular-resolution and sensitivity.

Cone search capability for table J/A+A/600/A4/list (List of fits cubes)

Identifier
DOI http://doi.org/10.26093/cds/vizier.36000004
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/600/A4
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/600/A4
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/600/A4
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/600/A4
Provenance
Creator Castro-Carrizo A.; Bujarrabal V.; Neri R.; Alcolea J.,Sanchez Contreras C.; Santander-Garcia M.; Nyman L.-A.
Publisher CDS
Publication Year 2017
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; Exoplanet Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics