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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



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ID: 559472.0, MPI für Astronomie / Publikationen_mpia
The Vega debris disc: A view from Herschel
Authors:Sibthorpe, B.; Vandenbussche, B.; Greaves, J. S.; Pantin, E.; Olofsson, G.; Acke, B.; Barlow, M. J.; Blommaert, J. A. D. L.; Bouwman, J.; Brandeker, A.; Cohen, M.; De Meester, W.; Dent, W. R. F.; di Francesco, J.; Dominik, C.; Fridlund, M.; Gear, W. K.; Glauser, A. M.; Gomez, H. L.; Hargrave, P. C.; Harvey, P. M.; Henning, Th; Heras, A. M.; Hogerheijde, M. R.; Holland, W. S.; Ivison, R. J.; Leeks, S. J.; Lim, T. L.; Liseau, R.; Matthews, B. C.; Naylor, D. A.; Pilbratt, G. L.; Polehampton, E. T.; Regibo, S.; Royer, P.; Sicilia-Aguilar, A.; Swinyard, B. M.; Waelkens, C.; Walker, H. J.; Wesson, R.
Language:English
Date of Publication (YYYY-MM-DD):2010
Title of Journal:Astronomy and Astrophysics
Journal Abbrev.:A&A
Volume:518
Start Page:id.L130
Review Status:Peer-review
Audience:Experts Only
Abstract / Description: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. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.
Free Keywords:stars: individual: Vega; instrumentation: photometers; methods: observational
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2010A%26A...518L.130... [ID No:1]
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