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21 - 26 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. mnr_20522_LR

    https://people.ast.cam.ac.uk/~wyatt/vw12.pdf
    30 Oct 2012: Fig. 2 indicates that this bifurcation value is a factor of2–20 times as high as the Solar system’s post-main-sequence escapeboundary.

  3. Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/jw12.pdf
    19 Jun 2012: Afteraround 15-20 kyr, the timescale for most particle orbits to completea precession cycle, this is no longer a significant effect. ... over 10 Myr is decreased by around 20 percentwhen Venus, Mars and Jupiter are added.

  4. midi_terr_sub3_nobold.dvi

    https://people.ast.cam.ac.uk/~wyatt/swh12.pdf
    24 Feb 2012: sub-integration.These profiles are taken at 110 EoN (to coincide with theresidual emission peaks at Q) and 20 EoN (perpendicularto the residual peaks). ... At 20 EoN and at both angles in the N band, theFWHMs of HD172555 are consistent with those

  5. ApJ409619o.dvi

    https://people.ast.cam.ac.uk/~wyatt/lwcm11.pdf
    23 Feb 2012: The prevalence ofdebris disks around Sun-like stars and more massive stars(20%–60%; Rieke et al. ... The η Corvi spectrum shows relativelystrong, moderate contrast features, indicative of the presence ofsmall (1 μm) to medium (20 μm)-sized grains.

  6. Observing Kepler stars with WISE

    https://people.ast.cam.ac.uk/~wyatt/kw12.pdf
    7 Jul 2012: Key words: planets and satellites: formation — stars:individual, HD 69830, BD 20 307,HD 172555,η Corvi, HIP 13642, KIC 7345479. ... HD 69830,HD 172555, BD 20 307,η Corvi, HD 165014, HD 169666,HD 15407A Beichman et al.

  7. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture13.pdf
    4 Nov 2012: We shall return to White Dwarfs in a subsequent lecture. 20.

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