Sibthorpe, B;
Vandenbussche, B;
Greaves, JS;
Pantin, E;
Olofsson, G;
Acke, B;
Barlow, MJ;
... Wesson, R; + view all
(2010)
The Vega debris disc: A view from Herschel.
Astronomy & Astrophysics
, 518
, Article L130. 10.1051/0004-6361/201014574.
Preview |
Text
sibthorpe_vega_aa14574-10.pdf - Published Version Download (251kB) | Preview |
Abstract
We present five band imaging of the Vega debris disc obtained using the Herschel Space Observatory. These data span a wavelength range of 70–500 μm with full-width half-maximum angular resolutions of 5.6–36.9”. The disc is well resolved in all bands, with the ring structure visible at 70 and 160 μm. Radial profiles of the disc surface brightness are produced, and a disc radius of 11” (~85 AU) is determined. The disc is seen to have a smooth structure thoughout the entire wavelength range, suggesting that the disc is in a steady state, rather than being an ephemeral structure caused by the recent collision of two large planetesimals.
Type: | Article |
---|---|
Title: | The Vega debris disc: A view from Herschel |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1051/0004-6361/201014574 |
Publisher version: | https://doi.org/10.1051/0004-6361/201014574 |
Language: | English |
Additional information: | This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions. |
Keywords: | stars: individual: Vega / instrumentation: photometers / methods: observational |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery-pp.ucl.ac.uk/id/eprint/10095322 |
Archive Staff Only
View Item |