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The Vega debris disc: A view from Herschel

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. Green open access

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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
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