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11 - 20 of 21 search results for TALK:PC53 20 |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. arX iv:1 403. 6186 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/mmek14.pdf
    2 Jul 2014: withthe general incidence of 20.2 2.0% from the DUNES sur-vey (Eiroa et al. ... 2013). PreviousSpitzer results for 45 FGK ex-oplanet hosts record an incidence of 20.87.0.

  3. Mon. Not. R. Astron. Soc. 000, 1–22 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pw14.pdf
    2 Jul 2014: x (au)100 50 0 50 100. z (au)20 0 20. Figure 1. ... These critical in-clinations were around 20 and 25 for ωplt = 90 and 45.

  4. Mon. Not. R. Astron. Soc. 000, 1–?? (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/mpwd15.pdf
    10 Dec 2014: 0. 10. 20. δ of. fset. ("). Figure 1. Continuum non-primary-beam-corrected image of the. ... 30. 60. 90. 120. -20 -15 -10 -5 0 5 10 15 20vhel - rv (km/s).

  5. arX iv:1 408. 4116 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kw14.pdf
    22 Aug 2014: Aug. 201. 4Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 20 August 2014 (MN LATEX style file v2.2). ... temperatureratios is in the 15-20 range (depending on the temperature ofthecool component).

  6. Constraining the Exozodiacal Luminosity Function of Main Sequence…

    https://people.ast.cam.ac.uk/~wyatt/mmsc14.pdf
    18 Oct 2014: Each. group contains 20 stars each, allowing a straightforward comparison of the observed distributions. ... hot excess (11), hot excess only (4), and stars with no infrared excess reported (20).

  7. arX iv:1 402. 1184 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/dawk14.pdf
    10 Feb 2014: 15-20% around Main Sequence stars, with increased frequency around younger stars (Su et al. ... function cannot simultaneously match the peak wavelength and the 20–70 µm slope, thus requiring.

  8. mn.dvi

    https://people.ast.cam.ac.uk/~wyatt/wfpb14.pdf
    23 Jan 2014: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 23 January 2014 (MN LATEX style file v2.2). Stochastic accretion of planetesimals onto white dwarfs:. constraints on the mass distribution of accreted material. from atmospheric pollution. M.

  9. Mon. Not. R. Astron. Soc. 000, 1–22 (2013) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/jwbv14.pdf
    11 Mar 2014: 2)moves. From Fig. 2 and the dependencies of Eqs. 16-20 we canalso make some simple general observations about non-sphericallysymmetric distributions of kick angles. ... Figure 2. Distributions of orbital elements for a set of 20,000 particles givena

  10. Five steps in the evolution from protoplanetary to debrisdisk ...

    https://people.ast.cam.ac.uk/~wyatt/wpkm15.pdf
    17 Dec 2014: To construct an unbiased sample we use thenearby 20 Myr β Pic moving group (BPMG; Zucker-man et al. ... as transition disks ranges from 10-20% (e.g., Muzerolle. et al. 2010; Furlan et al.

  11. Irwin06draft.dvi

    https://people.ast.cam.ac.uk/~wfcam/ukreview/Irwin06draft.pdf
    23 Jul 2014: 6.5 6.8 5.4 7.2 20 CDS 4.6. 6.5 6.2 6.6 6.0 5 CDS 4.5. ... This therefore predictsa 20% overestimate of the gain, and hence a 20% over-estimate of the QE coefficients.

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