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1 - 4 of 4 search results for `Watson A A` |u:people.ast.cam.ac.uk

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  2. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt
    2 Jul 2010: Since, as noted before, a sensible observing sequence precludes it being a problem. ... There has been a further shrinkage of staff at UKIRT. Tom Kerr is now our main contact with Watson the other UKIRT contact.

  3. arX iv:1 008. 0865 v2 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/cws10.pdf
    22 Aug 2010: This was then subtracted from the final. image to ensure a flat background. ... 2006), compared to a belt at 55AU with a width of50AU for HD191089.

  4. Are Debris Disks Self-Stirred?

    https://people.ast.cam.ac.uk/~wyatt/kw10.pdf
    19 Feb 2010: Weshow that there is no significant statistical difference between fractional excessesof A-stars. ... 5). We also assume that the central star acts like a black-body.

  5. arX iv:1 004. 0644 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/sw10.pdf
    6 Apr 2010: possibilitiesinclude dynamical scattering by a migrating planet, see e.g.Gomes et al. ... This source together with HD 31295 andHD 38206 are described in Appendix A.

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