M 2-9 ^12^CO and ^13^CO channel maps Virtual Observatory Resource

Authors
  1. Castro-Carrizo A.
  2. Bujarrabal V.
  3. Neri R.
  4. Alcolea J.,Sanchez Contreras C.
  5. Santander-Garcia M.
  6. Nyman L.-A.
  7. Published by
    CDS
Abstract

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.

Keywords
  1. planetary-nebulae
  2. radial-velocity
  3. radio-astronomy
Bibliographic source Bibcode
2017A&A...600A...4C
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/600/A4
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/600/A4
Document Object Identifer DOI
doi:10.26093/cds/vizier.36000004

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/600/A4
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/600/A4
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/600/A4
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/600/A4/list?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/600/A4/list?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/600/A4/list?

History

2017-03-17T07:43:58Z
Resource record created
2017-03-17T07:43:58Z
Created
2017-05-22T15:02:45Z
Updated

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