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19 Apr 2006: The new dust libration parameters were thenused to work out the spatial distribution of these grains. ... The new centrecan be derived by making the sum of the inward decaydue to P-R drag (eq.

14 Dec 2006: We have detected a new debris disk around the M0.5 dwarf GJ 842.2 at λ = 850 µm, providing evidence for cold dust at largedistance from this star (300 AU). ... 2005). Ourcontribution to establishing the statistics of debris disks aroundM-dwarfs

28 Nov 2006: NEW DEBRIS DISKS AROUND NEARBY MAIN-SEQUENCE STARS:IMPACT ON THE DIRECT DETECTION OF PLANETS.

19 Apr 2006: A&A 440, 937–948 (2005)DOI: 10.1051/0004-6361:20053391c ESO 2005. Astronomy&. Astrophysics. Spiral structure when setting up pericentre glow: possible giantplanets at hundreds of AU in the HD 141569 disk. M. C. Wyatt. UK Astronomy Technology Centre

19 Apr 2006: to theobservations of debris disks around other stars; and e) how these new results impactour assessment of whether systems like our own are common or rare compared to theensemble of normal ... Several new far–infrared studies were initiated with

19 Apr 2006: Mon. Not. R. Astron. Soc. 334, 589–607 (2002). Collisional processes in extrasolar planetesimal discs – dust clumpsin Fomalhaut’s debris disc. M. C. Wyatt and W. R. F. DentUK Astronomy Technology Centre, Royal Observatory, Blackford Hill,

19 Apr 2006: 1. INTRODUCTION. A new generation of astronomical instrumentations isnow making it possible to image the thermal emission fromthe disks of dust that surround some stars.