Images of Vega at 1.3mm

DOI

Previous studies have found that Vega is surrounded by an extended debris disc that is very smooth in the far infrared, but displays possible clumpiness at 850um and dust emission peaks at 1.3mm. We reobserved Vega at 1.3mm with PdBI to constrain its circumstellar dust distribution.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35319002
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/531/L2
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/531/L2
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/531/L2
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/531/L2
Provenance
Creator Pietu V.; Di Folco E.; Guilloteau S.; Gueth F.; Cox P.
Publisher CDS
Publication Year 2011
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy