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1 - 10 of 21 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 21 match some words.

  1. Results that match 1 of 2 words

  2. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090715.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090715.txt
    20 Jul 2009: 7. VISTA update Raw data has been received via Garching for up to and including June 24.

  3. /astro/data/upsand1/mpayne/PLANETESIMAL_DRIVEN_MIGRATION/plots/plot_31…

    https://people.ast.cam.ac.uk/~wyatt/pwt09.pdf
    3 Sep 2009: 0.24), while its mass has further doubled to 0.4M.Only a very small amount of additional migration is observed. ... 0.24. Similarly, the mass of theouter-most body also increases significantly as the surfacedensityand the surface density ratio are

  4. New Page 1

    https://people.ast.cam.ac.uk/~cdm/cdm_CV_130509.htm
    14 May 2009: Taught the Introductory Astrophysics Lecture course, 24 lectures, 1998-2001 inclusive, and Topics in Contemporary Astrophysics, 2002-6 and 2008-present. ... Ph.D Awarded: 24.4.87. 8. Student: C A Haniff, Admission Date: 1.10.84, Title: High resolution

  5. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/wbpc09.pdf
    25 Oct 2009: Rewriting equation 23 gives. Mlate = [1.471011 Imax/K]M 4/3? q13/3t1[(1e)13/3S(e)]1, (24).

  6. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_091119.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_091119.txt
    30 Nov 2009: within 24 hours of the final bit of data being taken.

  7. Craig  Mackay

    https://people.ast.cam.ac.uk/~cdm/cdm_pub_list_130509.htm
    14 May 2009: ApJ, 270, 342 (1983). 24. Mackay, C.D. and Astill, D.M., CCD Development at Cambridge, England'. ... 31. Mackay, C.D., CCDs in Astronomy'. Ann. Rev. Ast. And Astrophys., 24, 255, 1986.

  8. 11626.dvi

    https://people.ast.cam.ac.uk/~wyatt/swh09.pdf
    23 Jun 2009: June 23, 2009. Resolving the hot dust around HD69830 and η Corvi with MIDI andVISIR. R. Smith1, M.C. Wyatt1, and C.A. Haniff2. 1 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0AHe-mail:rsed@ast.cam.ac.uk. 2

  9. Debris disk dynamical theory Mark Wyatt Institute of Astronomy, ...

    https://people.ast.cam.ac.uk/~wyatt/MarkWyatt_Spitzer2008Conference.pdf
    12 Jan 2009: Spitzer imaging of Vega disk. 850µm (Holland et al.). 24 and 70µm (Su et al. ... Diameter, D. σ(D), AU2. Dmin. Dmax. Evolution of size distribution. Steady-state evolution explains 24 and 70µm stats.

  10. lecture7_debrisdiskmod

    https://people.ast.cam.ac.uk/~wyatt/lecture7_debrisdiskmod.pdf
    12 Feb 2009: The largest fragment in a collision, flr = Mlr/M is given by Q < QD flr = 1 – 0.5 (Q/QD) Q > QD flr = 0.5(QD/Q)1.24.

  11. Planets and Debris Disks: Results from a Spitzer/MIPS Search ...

    https://people.ast.cam.ac.uk/~wyatt/bbcr09.pdf
    15 Sep 2009: 24 µm, indicative of warm dust in the inner system analogous to that produced. ... 16 –. wavelength (13 at 70 µm, plus HD 69830 at only 24 µm).

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