Images of Vega at 1.3mm Virtual Observatory Resource

Authors

1. Pietu V.
2. Di Folco E.
3. Guilloteau S.
4. Gueth F.
5. Cox P.

Published by

CDS

Abstract

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.

Keywords

1. variable-stars
2. millimeter-astronomy
3. photometry
4. submillimeter-astronomy

Bibliographic source Bibcode

2011A&A...531L...2P

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/531/L2

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/531/L2

Document Object Identifer DOI

doi:10.26093/cds/vizier.35319002

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/531/L2
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/531/L2
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/531/L2

IVOA Table Access TAP

https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).