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1 - 10 of 29 search results for katalk:za33 24 |u:people.ast.cam.ac.uk where 0 match all words and 29 match some words.

  1. Results that match 1 of 2 words

  2. Basic Debris Disk Model

    https://people.ast.cam.ac.uk/~wyatt/wyatt_uf07.pdf
    24 Apr 2007: 2005):. F 24/. F. Steady-state planetesimal belt evolution. The size distribution in a collisionalcascade is to first order described by a power law. ... Wyatt et al. (2007a). This model accurately reproduces the fraction of stars in different age bins

  3. wyatt

    https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf
    18 Jun 2007: Steady-state evolution explains 24 and 70µm stats. Wyatt et al. (2007b).

  4. Microsoft PowerPoint - wyattpub

    https://people.ast.cam.ac.uk/~wyatt/wyatt_kobe06.pdf
    24 Apr 2007: stars at 24,70,160μm• Akari (2006-) currently doing all-sky survey 2-180μm• Herschel (2008-) observations at 60-670μm• Spica (2017+) planned 5-200μm. ... Structure is wavelength dependent!850μm. (Holland et al. 2006)24 and 70μm. (Su et al.

  5. Submitted to ApJ, 3 January 2007, accepted 22 March ...

    https://people.ast.cam.ac.uk/~wyatt/wssr07.pdf
    23 Mar 2007: The 150t1age line delineatingthe upper envelope of the 24 µm detections (Rieke et al. ... 4.2.1. Sample of 46 A star disks detected at 24 and 70µm.

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

    https://people.ast.cam.ac.uk/~wyatt/wcg07.pdf
    18 Jul 2007: L. Arnold, F. Bouchy, C. Moutou (Paris: FrontierGroup), 24. Boss A., 2002, ApJ, 567, L149Butler R.

  7. arX iv:0 704. 3369 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/mlpw07.pdf
    26 Apr 2007: 24). In Figure 4 we compare models having5 MJ between the planets with and without disc matter lo-cated inside the inner planet. ... The mass distributionfollows equation (24) and the outer disc mass is varied bychanging parameter Σ0out.

  8. MASS AND TEMPERATURE OF THE TWA 7 DEBRIS DISK ...

    https://people.ast.cam.ac.uk/~wyatt/mkw07.pdf
    3 Jul 2007: 1), which fits the three longest wavelength fluxes, but cannotreproduce the 24 m flux. ... 1999, ApJ, 512, 377Hildebrand, R. 1983, QJRAS, 24, 267Holland, W. S., et al.

  9. 842 Publications of the Astronomical Society of the Pacific, ...

    https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf
    18 Sep 2007: stellar luminosities. TheA stars (dark blue) are a sample of 46 detected at both 24 and 70mm (Wyattet al. ... A0, 3.6–24.8 pc for G0, and 1.8–8.6 pc for M0.

  10. hd113766_dust_25Sep2007

    https://people.ast.cam.ac.uk/~wyatt/lcwm08.pdf
    5 Oct 2007: excess 24 and 70 µm flux. In their follow-on study, which provided the data used in this work,. ... silicate emission features at 9.8, 11.2, 16.2, 19, 24, and 34 µm.

  11. arX iv:0 704. 0873 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf
    18 Apr 2007: hot Jupiter –0.08 to 0.39 1.7–5 [500–1600] 70–200 1 % 2 1 %cool Jupiter –0.44 to 0.40 0.24–1.7 [75–500] ... 200 8 % 9 (5–11) %. planet & debris –0.13 to 0.27 0.10–0.24 [30–75] 5–30 5 % 3 1 %debris –0.52 to 0.18

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