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21 - 25 of 25 search results for `Watson et al` |u:people.ast.cam.ac.uk

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  2. arX iv:1 511. 0591 9v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf
    25 Nov 2015: Continued. c 2002 RAS, MNRAS000, 1–18. 6 Z. H. Draper et al. ... of the disk is morewidely distributed than a simple ring (Booth et al.

  3. TLA_large

    https://people.ast.cam.ac.uk/~wyatt/tgmk14.pdf
    4 Dec 2014: They are less massive thanprotoplanetary discs ( 1 M of dust; Panić et al. ... 2008), Monnier et al. (2012, Vega), Mamajek (2012,Fomalhaut) and Zuckerman et al.

  4. arX iv:1 403. 6186 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/mmek14.pdf
    2 Jul 2014: 2001; Mayor & Queloz 2012) or transit surveys e.g. CoRoT(Auvergne et al. ... 2010; Rodler et al. 2011; Giacobbe et al. 2012;Anglada-Escudé & Tuomi 2012).

  5. Observations, Modeling and Theory of Debris Disks Brenda C. ...

    https://people.ast.cam.ac.uk/~wyatt/mkwb14.pdf
    7 Jan 2014: 2006) sur-veys and Herschel DEBRIS2 (Matthews et al. 2013b) andDUNES3 (Eiroa et al. ... stars are statistically indistinguishable,a result supported by DUNES data (Eiroa et al.

  6. arX iv:1 701. 0656 8v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/kkpr17.pdf
    5 May 2017: As argued by de Wit et al. [40] a picture is emerging in which RZ Pscis surrounded by a massive young version of our own asteroid belt, in which planetesimalsare continually ... 675 1.5] 1.05, where anextinction of 0.3 per unit airmass was used, derived

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