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1 - 10 of 13 search results for katalk:za33 24 |u:people.ast.cam.ac.uk where 0 match all words and 13 match some words.

  1. Results that match 1 of 2 words

  2. ib2016michaelmas.dvi

    https://people.ast.cam.ac.uk/~cat/ib.pdf
    3 Oct 2016: Quantum Mechanics (16 lectures, 3 supervisions)Miss A. D. Ming (adk33@cam.ac.uk). Methods (24 lectures, 4 supervisions)David Baker (dib27@cam) or Oliver Petrie (op246@cam.ac.uk). ... Analysis II (24 lectures, 4 supervisions)Dr M. J. Donald (mjd1014@cam.ac

  3. ms.dvi

    https://people.ast.cam.ac.uk/~wyatt/wmke16.pdf
    10 Nov 2016: M. Using the previous imagingconstraints on ωΣ0 with the SED constraint on (1 ω)Σ0,we find the albedo, ω =0.13–0.24. ... radius (rin, au) 28.5 (26.8, 30.4) 27.6 (26.9, 28.2) 25.0 (24.1, 25.8)”Birth” ring width (r, au) 5.0 (1.8,

  4. vpfit10.4.dvi

    https://people.ast.cam.ac.uk/~rfc/vpfit10.4.pdf
    5 Oct 2016: H I 0.29051 0.0000221 4.5144 0.00 0.00E00! 2. H I 0.56100 0.0004240 24.5479 0.00 0.00E00! ... HE0515c1.fits 1 3691.3777 3693.0135. 24. %% HE0515c2.fits 1 3697.6064 3699.1730.

  5. MNRAS 000, 1–6 (2016) Preprint 13 July 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/agwk16.pdf
    13 Jul 2016: 203850058 16253849-2613540 16:27:06.596 -24:41:48.84 Oph M6 2700 3.0 Full 2.88 0.18 Q.

  6. Astronomy & Astrophysics manuscript no. letter_HD206893 c©ESO…

    https://people.ast.cam.ac.uk/~wyatt/mhcc16.pdf
    2 Dec 2016: mass in the range 24 to 73MJup for an age of the system in the range 0.2 to 2 Gyr.

  7. Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf
    21 Jul 2016: 32 200 (4) u.l. u.l.HD95418 A1V 24 320 (9) u.l.HD10939 A1V 62 350 (M) u.l.HD216956 Fomalhaut A4V 7.7 440 (10) u.l. ... 4(1.8) 0.5 24.3(0.4) 1.7(0.4) 2.68(0.72) 0.80(0.17) < 1.5F(OI) 245(5) 1.5 7 7.3

  8. arX iv:1 604. 0828 6v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/mcbe16.pdf
    29 Apr 2016: 1 24.3 11.3 24.9 11.2 21.3 1.17 51.1 15.3. ... Southern Ratio 0.97 0.17 36.4 13.0 24.9Control Ratio 1.16 0.22 9.8 9.6.

  9. Space Science Reviews manuscript No.(will be inserted by the ...

    https://people.ast.cam.ac.uk/~wyatt/wj16.pdf
    15 Mar 2016: For this reason Fig. 5, which showsthe predicted brightness evolution of giant impact debris at two wavelengths12 and 24 µm at which stars are commonly observed, shows that evolutionfor two different ... This has the benefit of resulting in aconstant

  10. MNRAS 000, 1–12 (2015) Preprint 12 May 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mmsw16.pdf
    17 May 2016: 1 http://www.ita.uni-heidelberg.de/dullemond/software/radmc-3d/. 0.06. 0.09. 0.12. 0.15. 0.18. h. 20 22 24 26. ... We can then extrapolate this to obtain a collisionallifetime of mm-sized grains of 24 103 yr ( 34 orbits).

  11. Mon. Not. R. Astron. Soc. 000, 1–16 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/kwcp16.pdf
    7 Jun 2016: Mon. Not. R. Astron. Soc. 000, 1–16 (2002) Printed 7 June 2016 (MN LATEX style file v2.2). A self-consistent model for the evolution of the gasproduced in the debris disc of β Pictoris. Q. Kral?, M. Wyatt, R. F. Carswell, J. E. Pringle, L. Matrà

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