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21 - 30 of 42 search results for katalk:PC53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 42 match some words.

  1. Results that match 1 of 2 words

  2. aa2073.dvi

    https://people.ast.cam.ac.uk/~wyatt/wyat05b.pdf
    19 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

  3. NEW DEBRIS DISKS AROUND NEARBY MAIN-SEQUENCE STARS:IMPACT ON THE ...

    https://people.ast.cam.ac.uk/~wyatt/bbsg06.pdf
    28 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.

  4. Dust_in_the_Debris_Disk_Around_HD69830_09Nov2006

    https://people.ast.cam.ac.uk/~wyatt/lbbw07.pdf
    16 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.

  5. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt
    6 Nov 2006: The UK VDFS review was held on 24/25 October at Cambridge.

  6. Evolution of Circumstellar Disks Around Normal Stars:Placing Our…

    https://people.ast.cam.ac.uk/~wyatt/mbww07.pdf
    19 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

  7. SUBMILLIMETER IMAGES OF A DUSTY KUIPER BELT AROUND � ...

    https://people.ast.cam.ac.uk/~wyatt/wgdc05.pdf
    19 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.

  8. Oxford Meeting

    https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt
    15 Apr 2006: B440022.122.24.82.6. V550021.321.49.63.5. R600020.420.817.93.9. I750019.520.035.25.2. Z890018.218.7117.26.3. J12,50016.016.9609.39.3.

  9. THE ASTROPHYSICAL JOURNAL, 530 : 329È341, 2000 February 102000. ...

    https://people.ast.cam.ac.uk/~wyatt/tfpk00.pdf
    19 Apr 2006: d)Logarithmic 18.2 km levels : 8.0, 10.6, 13.9, 18.4, 24.3, 32.1, 42.3, 55.9, and 73.7.

  10. ��������� ��� ������������������� ������� ������� ��!�� #"$��…

    https://people.ast.cam.ac.uk/~wyatt/wyat99.pdf
    19 Apr 2006: 2/)C"C$ )!1-N. 2#1 D 4'@! 24"BC #" 1 9 #"S243! S'@ #3<TU,3- #"D32#!24"24,! :<')("!-! ... $-"8 =H0,"80 N,'<Q ; 3j Y-. ) ,"8 2MP 24 3j ;2)!

  11. Submitted to ApJ 16 July 2006, Accepted 3 October ...

    https://people.ast.cam.ac.uk/~wyatt/wsgb07.pdf
    2 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).

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