22-GHz water maser clouds

DOI

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.

Cone search capability for table J/A+A/546/A16/stars (Properties of the stars)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35460016
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/546/A16
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/546/A16
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/546/A16
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/546/A16
Provenance
Creator Richards A.M.S.; Etoka S.; Gray M.D.; Lekht E.E.; Mendoza-Torres J.E.,Murakawa K.; Rudnitskij G.; Yates J.A.
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; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy