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https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt6 Nov 2006: The UK VDFS review was held on 24/25 October at Cambridge. -
Data Flow System Document Title: VISTA Data Reduction Library ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0010.pdf28 Sep 2006: 0001, issue 3.2 2005-02-24. [RD 3] VISTA Science Requirements Document, VIS-SPE-VSC-00000-0001, issue. ... 13 / kk leads to a relative area of. )41()31).(1( 222 rkrkrk ′′′ (2-24). -
Submitted to ApJ 16 July 2006, Accepted 3 October ...
https://people.ast.cam.ac.uk/~wyatt/wsgb07.pdf2 Nov 2006: 0.5M2v2rel = M1Q? D whereas DD03 define S to be the specific bind-ing energy of the two objects (giving their equation 24). ... dNc(D > Dpb)/dt = 1000r13/3(dr/r)t2ageDcD. 3pb. M4/3? Q? D. 5/6e5/3, (24). -
SUBMILLIMETER IMAGES OF A DUSTY KUIPER BELT AROUND � ...
https://people.ast.cam.ac.uk/~wyatt/wgdc05.pdf19 Apr 2006: The total measured flux was 1:51 0:24 Jy (S=N 7);the dominant uncertainty in this flux estimate is the calibrationuncertainty. -
Evolution of Circumstellar Disks Around Normal Stars:Placing Our…
https://people.ast.cam.ac.uk/~wyatt/mbww07.pdf19 Apr 2006: Surprisingly, however, the 24 and 70 µm images of Vegaactually have larger radii than the submillimeter ring or mil-limeter clumps (Su et al., 2005). ... Emission (Additional)Vega A0 200 >90 23,24,25 Eridani K2 <1000 60 26,27η Corvi F2 1000 100 28τ -
aa2073.dvi
https://people.ast.cam.ac.uk/~wyatt/wyat05b.pdf19 Apr 2006: A&A 433, 1007–1012 (2005)DOI: 10.1051/0004-6361:20042073c ESO 2005. Astronomy&. Astrophysics. The insignificance of P-R drag in detectableextrasolar planetesimal belts. M. C. Wyatt. UK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9 -
Placing Our Solar System in Context:[A 12 step program ...
https://people.ast.cam.ac.uk/~wyatt/mmeyer_etal_ppv.pdf19 Apr 2006: MIR.but more common around stars < 100 Myr. MIPS 24 um image of Vega disk. ... MIPS-24 MIPS-70. MIPS-160 JCMT-450CSO-350. HST. Do Stars with Inner Planets (< 5 AU) Also Have Kuiper Disks? -
Dust_in_the_Debris_Disk_Around_HD69830_09Nov2006
https://people.ast.cam.ac.uk/~wyatt/lbbw07.pdf16 Nov 2006: 2.46 Diopside (CaMgSi2O6) 0.05 3.3 216 0.075 340 1.53 Carbonates Magnesite (MgCO3) 0.07 3.1 84 0.24 370 1.54 Dolomite (CaMgC2O6) d ... 12 and 25 um photometry (Mannings and Barlow 1998), and Spitzer 24 and 70 um photometry. -
NEW DEBRIS DISKS AROUND NEARBY MAIN-SEQUENCE STARS:IMPACT ON THE ...
https://people.ast.cam.ac.uk/~wyatt/bbsg06.pdf28 Nov 2006: a Significance of 24 m excess (eq. [1]).b Significance of 70 m excess (eq. ... 2000). Finally,HD 23249 and HD 55892 have 2 < 24 < 3 and 70 < 2. -
Mon. Not. R. Astron. Soc. 334, 589–607 (2002) Collisional ...
https://people.ast.cam.ac.uk/~wyatt/wd02.pdf19 Apr 2006: 25 1.24 0.6 IRAS60 9.80 0.62 IRAS60 7.51 0.92 ISO80 8.86 0.87 ISO100 10.95 0.66 IRAS100 11.04 2.0 ISO120
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