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21 - 30 of 39 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 39 match some words.

  1. Results that match 1 of 2 words

  2. 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.

  3. ESO Public Surveys Proposal Form Phase 1 Title: The ...

    https://people.ast.cam.ac.uk/~rgm/vhs/PS-VHS-v4p2-Appendix-B-PSP-Response.pdf
    9 Oct 2006: ESO Public Surveys Proposal Form Phase 1. reaching 10sigma limits[AB mags] in g, r, i and z of 24.1, 23.7, 23.3 and 22.6 respectively. ... with 10sigma limit of 24.6, 24.1, 24.3 and 23.9.

  4. 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

  5. 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.

  6. 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.

  7. ��������� ��� ������������������� ������� ������� ��!�� #"$��…

    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)!

  8. 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).

  9. arX iv:a stro -ph/ 0311 593 v1 26 N ...

    https://people.ast.cam.ac.uk/~wyatt/sdw04.pdf
    19 Apr 2006: 32 0.02 0.13 0.04 < 0.5HD207129 0.60 0.03 0.15 0.02 0.31 0.04 < 0.24. ... However, sub-mm observations made withSCUBA on the JCMT indicate a diameter of 24 3 arc-sec (Holland et al.

  10. 58419 1321..1340

    https://people.ast.cam.ac.uk/~wyatt/wyat03b.pdf
    19 Apr 2006: Crosses show the location of a planetesimal in the different resonances (2 : 1, 5 : 3, 3 : 2, and 4 : 3,from top to bottom) at intervals of 1/24 of the ... l1:24. e0:42. ; ð33Þ. D5 :3h i 13:2 þ 290:0=l1:33. ; ð34Þ.

  11. Mon. Not. R. Astron. Soc. 334, 589–607 (2002) Collisional ...

    https://people.ast.cam.ac.uk/~wyatt/wd02.pdf
    19 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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