TX Psc ALMA CO(2-1) images

DOI

We observed the carbon-rich asymptotic giant branch (AGB) star TX Piscium (TX Psc) with ALMA in CO(2-1) emission to investigate the circumstellar envelope (CSE) and mass-loss history of this object. Previous observations with Herschel in the far infrared have shown a ring-like structure in dust emission (2011A&A...532A.135J). Our molecular gas observations of the CO(2-1) emission line cover this structure with significantly higher spatial resolution to investigate its origin.

Cone search capability for table J/A+A/621/A50/list (List of fits images)

Associated data

Identifier
DOI http://doi.org/10.26093/cds/vizier.36210050
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/621/A50
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/621/A50
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/621/A50
Related Identifier https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/A+A/621/A50
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/621/A50
Provenance
Creator Brunner M.; Mecina M.; Maercker M.; Dorfi E.A.; Kerschbaum F.; Olofsson H.,Rau G.
Publisher CDS
Publication Year 2019
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; Stellar Astronomy