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11 - 20 of 26 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 26 match some words.

  1. Results that match 1 of 2 words

  2. arX iv:1 201. 1911 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwsd12.pdf
    12 Jan 2012: 20. DE. C o. ffset. ("). -0.10. 0.04. 0.18. 0.32. 0.46. ... 0. 10. 20. DE. C o. ffset. ("). -0.08. 0.00. 0.08.

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

    https://people.ast.cam.ac.uk/~wyatt/bksm12.pdf
    5 Oct 2012: These 9 stars constitute the full sample of resolvedA star discs between 20 and 40 pc. ... PSF fit500 20.30.4 0.210.00 20.00.4 PSF fit.

  4. Draft version December 10, 2012Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/bmkb12.pdf
    10 Dec 2012: 2000)V magnitude 4.25 Balona et al. (1994)Distance (pc) 20.46 0.15 Phillips et al. ... 6 Broekhoven-Fiene et al. 0 5 10 15 20 25Semimajor axis (arcsec).

  5. cv.dvi

    https://people.ast.cam.ac.uk/~gpe/cv.pdf
    24 Jan 2012: J. Supp., 107, 20 1. [R97] Power Spectrum Analysis of the Stromlo-APM Redshift Survey. ... 20 authors, 2000, Astro. Lett. and Communications, 37, 161. [R138] Simulations of Deep Pencil-Beam Redshift Surveys N.

  6. mnr_21298_LR

    https://people.ast.cam.ac.uk/~wyatt/wksm12.pdf
    7 Nov 2012: correction for a 20 arcsec aperture quoted by the PACS team2 of 17,20 and 26 per cent. ... sensitiv-ity for an extended source at 3.7 arcsec radius of 20.0 mag arcsec2.

  7. arX iv:1 211. 4898 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/lmsk12.pdf
    24 Nov 2012: This data filtering results in the sourceflux density being underestimated by 20 5% as discussedin detail by Kennedy et al. ... 100µm 0.99 408 2.2 1.2 312214 55 (100) 2 α 0 3.50.51 60 110 20.

  8. Dynamical effects of stellar massloss on a Kuiperlike belt

    https://people.ast.cam.ac.uk/~wyatt/bmw11.pdf
    22 May 2012: Of the values of initialeccentricity and inclination tested here, the numerical simulationwith emax = 0.2 and imax = 20 scatters the most test particles.This implies that an analytic formulation for the ... A further numerical simulation with emax = 0.2

  9. arX iv:1 205. 0004 v2 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/fgwg12.pdf
    9 Oct 2012: 4 Ju. n 20. 12Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 15 June 2012 (MN LATEX style file v2.2).

  10. 1 A SELF-CONSISTENT MODEL OF THE CIRCUMSTELLAR DEBRIS CREATED ...

    https://people.ast.cam.ac.uk/~wyatt/jlcm12.pdf
    23 Oct 2012: μm is attributed to the Si-O bond vibration of amorphous silica and, along with a secondary 20. ... 20. described at the beginning of this section. Although, the submicron obsidian grains with.

  11. arX iv:1 201. 3622 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/ramb12.pdf
    19 Jan 2012: Jy. Start5 Myr42.8 Myr43.5 Myr100 Myr. 0 20 40 60 80 100Time (Myr). ... 0 5 10 15 20 25 30Width of stable zone (mutual Hill radii).

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