22-GHz water maser clouds Virtual Observatory Resource

Authors
  1. Richards A.M.S.
  2. Etoka S.
  3. Gray M.D.
  4. Lekht E.E.
  5. Mendoza-Torres J.E.,Murakawa K.
  6. Rudnitskij G.
  7. Yates J.A.
  8. Published by
    CDS
Abstract

Cool, evolved stars undergo copious mass loss but the detailed mechanisms and the form in which the matter is returned the ISM are still under debate. We investigated the structure and evolution of the wind at 5 to 50 stellar radii from Asymptotic Giant Branch and Red Supergiant stars.

Keywords
  1. supergiant-stars
  2. astrophysical-masers
  3. radio-astronomy
Bibliographic source Bibcode
2012A&A...546A..16R
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/546/A16
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/546/A16
Document Object Identifer DOI
doi:10.26093/cds/vizier.35460016

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/546/A16
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/546/A16
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/546/A16
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/546/A16/stars?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/546/A16/stars?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/546/A16/stars?

History

2012-09-27T09:26:23Z
Resource record created
2012-09-27T09:26:23Z
Created
2022-05-11T08:54:42Z
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