Search

19 Apr 2006: Our 850 mm map, obtained with the Submillimeter Common-UserBolometric Array on the James Clerk Maxwell Telescope, shows three peaks of emission at the 2.5 mJy levelin the vicinity of

19 Apr 2006: 1999) wasused on the James Clerk Maxwell Telescope (JCMT) toobtain deep simultaneous images of Fomalhaut at wave-lengths of 450 and 850 lm.

19 Apr 2006: 1999) at the James Clerk Maxwell Telescope wasused to observe τ Ceti in 2001 September and November, for a totalintegration time of 13.3 h.

19 Apr 2006: 2 OBSERVATIONS. Sub-mm observations were made using the SCUBA bolome-ter array on the James Clerk Maxwell Telescope. ... Details of Maxwell-Garneteffective medium theory, and the methods used to calculateabsorption efficiencies are discussed in Bohren &

19 Apr 2006: 2. OBSERVATIONS. 2.1. Submillimeter. The submillimeter observations of Corvi were made usingthe Submillimeter Common-User Bolometer Array (SCUBA)at the James Clerk Maxwell Telescope (JCMT).

19 Apr 2006: The 850 µm map of Vega obtained by Holland et al.(1998) with the Submillimeter Common-User Bolome-ter Array (SCUBA) on the James Clerk Maxwell Tele-scope shows an extended,

19 Apr 2006: 1.Recently the structure of the disc was mapped at both 450 and850 µm using SCUBA at the James Clerk Maxwell Telescope(JCMT) (Holland et al. ... We usethe optical constants for each of the components taken from Li &Greenberg (1997, 1998) and compute

19 Apr 2006: RESONANT TRAPPING OF PLANETESIMALS BY PLANET MIGRATION: DEBRIS DISK CLUMPSAND VEGA’S SIMILARITY TO THE SOLAR SYSTEM. M. C. WyattUK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9 3HJ, UK; wyatt@roe.ac.uk. Received 2003 June 11;