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The β Pictoris disk imaged by Herschel PACS and SPIRE

Title: The β Pictoris disk imaged by Herschel PACS and SPIRE
Authors: Vandenbussche, B; Sibthorpe, B; Acke, B; Pantin, E; Olofsson, G; Waelkens, C; Dominik, C; Barlow, MJ; Blommaert, JADL; Bouwman, J; Brandeker, A; Cohen, M; De Meester, W; Dent, WRF; Exter, K; Di Francesco, J; Fridlund, M; Gear, WK; Glauser, AM; Gomez, HL; Greaves, JS; Hargrave, PC; Harvey, PM; Henning, T; Heras, AM; Hogerheijde, MR; Holland, WS; Huygen, R; Ivison, RJ; Jean, C; Leeks, SJ; Lim, TL; Liseau, R; Matthews, BC; Naylor, DA; Pilbratt, GL; Polehampton, ET; Regibo, S; Royer, P; Sicilia-Aguilar, A; Swinyard, BM; Walker, HJ; Wesson, R
Source: Astronomy & Astrophysics , 518 , Article L133. (2010)
Publisher Information: EDP SCIENCES S A
Publication Year: 2010
Collection: University College London: UCL Discovery
Subject Terms: stars: early-type / planetary systems / circumstellar matter / stars: individual: β Pic
Description: We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V star β Pic. The disk is well resolved in the PACS filters at 70, 100, and 160 μm. The surface brightness profiles between 70 and 160 μm show no significant asymmetries along the disk, and are compatible with 90% of the emission between 70 and 160 μm originating in a region closer than 200 AU to the star. Although only marginally resolving the debris disk, the maps obtained in the SPIRE 250–500 μm filters provide full-disk photometry, completing the SED over a few octaves in wavelength that had been previously inaccessible. The small far-infrared spectral index (β = 0.34) indicates that the grain size distribution in the inner disk (
Document Type: article in journal/newspaper
File Description: text
Language: English
Relation: https://discovery.ucl.ac.uk/id/eprint/10095320/
Availability: https://discovery.ucl.ac.uk/id/eprint/10095320/1/vandenbussche_betapic_aa14626-10.pdf; https://discovery.ucl.ac.uk/id/eprint/10095320/
Rights: open
Accession Number: edsbas.5463F933
Database: BASE