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NEW DEBRIS DISKS AROUND NEARBY MAIN-SEQUENCE STARS:IMPACT ON THE ...
https://people.ast.cam.ac.uk/~wyatt/bbsg06.pdf28 Nov 2006: Typicaldistances range from 10 to 20 pc, closer for M and K stars andfarther for earlier spectral types. ... Stellar fluxes are measured within an aperture of 10 pixels(=1200), with a background annulus from 10 to 20 pixels. -
ApJ accepted, 7 November 2005Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/wyat06.pdf19 Apr 2006: 95.3 0.20 0.01 - 0.032.5 300 95.3 0.12 0.005 - 0.03. ... Since just 5% of the sub-mm emissioncomes from grains either < 300 µm or > 20 cm in diam-eter, with roughly equal weightings in this range towarddifferent. -
arX iv:a stro -ph/ 0601 592 v1 26 J ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/hewettetal.pdf28 Sep 2006: 3.238 1.000 4.193 1.548 -1.018 0.194 -0.272 0.073 0.110 20.0 2 8.0 386 3.53. ... 5.172 0.640 3.379 1.475 -0.390 -0.367 -0.293 0.076 0.132 16.3 20 9.0 686 4.66. -
58419 1321..1340
https://people.ast.cam.ac.uk/~wyatt/wyat03b.pdf19 Apr 2006: 1.41 210 20 1.0 0.2 1.84 0.02 0.20 0.08 0.042 : 1. ... 20. No. significant correlation could be found of D with either l orh for any of the resonances. -
Mon. Not. R. Astron. Soc. 334, 589–607 (2002) Collisional ...
https://people.ast.cam.ac.uk/~wyatt/wd02.pdf19 Apr 2006: ii) Collisional lifetimearguments imply that the collisional cascade starts with planetesimals 1.5–4 km in diameter,and so has a mass of 20–30 M. ... a 125-au radius ring inclined at 20 to the line of sight. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060612.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060612.txt18 Jul 2006: The total archive is about 20-25 Tbytes in size and has been backed up onto tape (100 Ultrium LTO-II tapes). ... These will be further discussed at the VISAS meeting in Edinburgh (20/21 June) which JRL will be attending to represent CASU. -
PDF/36/aa3391-05.pdf.url
https://people.ast.cam.ac.uk/~wyatt/wyat05c.pdf19 Apr 2006: 1). For example, Fig. 2 shows the complex ec-centricities of planetesimals that are at a = 1.4, 1.45 and 1.5aplat 20 equal timesteps ending at a time of ... Assuming the planet wasintroduced when the star (of mass 2.5 M) was born 5 Myr ago,this gives a -
VDF-WFA-VSA-004-I1.dvi
https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-WFA-VSA-004-I1.pdf29 Sep 2006: 20 Aperture flux 1 Aperture_flux_1 ADU. 21 Aperture flux 1 error Aperture_flux_1_error ADU. ... TUNIT40 = ’ADU ’ / physical unit of field. VDF-WFA-VSA-004, Draft 1.0, September 2006 20. -
Data Flow System Document Title: Cambridge Reduction and Analysis ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0017.pdf29 Sep 2006: 18 4.3 Triage. 19 4.4 Software. 20 4.5 Hardware. 21. 4.5.1 Processing Power. ... Doc: VIS-SPE-IOA-20000-0017 Issue: 1.0 Date: 2006-09-28. VISTA Data Flow. System. Cambridge Reduction and Analysis Pipeline Page: 20 of 23. -
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https://people.ast.cam.ac.uk/~wyatt/wyat99.pdf19 Apr 2006: 8 G'4-5:20"&. / -$>= JLKNKMK. '," ;"8 0 "8 2(4 / 18! ... 838 Y=,"9))-/g" ,R35! 4$6 0 Y "& 3! 4" >2)! - B" 20"!
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