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1 - 10 of 15 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 15 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: well. These considerations motivate us to choose f 0in increments of 30 from 0 to 330, supplemented by f 0 = [160,170, 190, 200]. ... cos 1(7/9) 160 and 360 f crit 200, which, for runaway mass loss, bound the region in which theeccentricity must

  3. midi_terr_sub3_nobold.dvi

    https://people.ast.cam.ac.uk/~wyatt/swh12.pdf
    24 Feb 2012: Mon. Not. R. Astron. Soc. 000, 1–22 (2011) Printed 24 February 2012 (MN LATEX style file v2.2). Resolving the terrestrial planet forming regions of. HD113766 and HD172555 with MIDI. R. Smith1,2, M. C. Wyatt2 and C. A. Haniff31Astrophysics Group,

  4. arX iv:1 201. 3622 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/ramb12.pdf
    19 Jan 2012: Each simulation was integrated for100-200 million years using the hybrid version of the Mercurycode (Chambers, 1999) with a 6 day timestep. ... 0.4. 0.8 200 Myr. Semimajor Axis (AU). Ecc. entr. icity. Log(Water Mass Fraction).

  5. ApJ409619o.dvi

    https://people.ast.cam.ac.uk/~wyatt/lwcm11.pdf
    23 Feb 2012: 2004) in amanner identical to that used for the 200 stars of the SPeX CoolStar library (Rayner et al. ... 3.2 200 0.11 350 1.62Diopside (CaMgSi2O6) 0.05 3.3 216 0.08 350 1.32.

  6. The Astrophysical Journal, 701:2019–2032, 2009 August 20…

    https://people.ast.cam.ac.uk/~wyatt/lcwm09.pdf
    1 Aug 2012: The mass of fine dust is 4 1019–2 1020 kg, equivalentto a 150–200 km radius asteroid. ... a very large particle dust population (a > 100 μm), radiatingas blackbodies at 200 K.

  7. Searching for Saturn's Irregular Satellite Swarm with Spitzer

    https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf
    29 Jun 2012: Stansberry. OFF ON IE IW. -600 -400 -200 0 200 400 600offset (Saturn radii). ... 400. -200. 0. 200. 400. offs. et (. Sat. urn. radi.

  8. arX iv:1 208. 1759 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwsp12.pdf
    9 Oct 2012: Coplanar Circumbinary Debris Disks 11. 0 50 100 150 200 250 300Semi-major axis (AU).

  9. arX iv:1 201. 1911 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwsd12.pdf
    12 Jan 2012: 57,PA = 3171 , ρ = 1.200.014”). ... An object in such an orbit would havea period of at least 200 years, so could not have been detectednear the star in 2005 and be outside the NIRC2 field of

  10. Observing Kepler stars with WISE

    https://people.ast.cam.ac.uk/~wyatt/kw12.pdf
    7 Jul 2012: arX. iv:1. 207. 0521. v1 [. astr. o-ph. EP. ] 2. Jul 2. 012. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 5 July 2012 (MN LATEX style file v2.2). Confusion limited surveys: using WISE to quantify the rarit y ofwarm dust around Kepler stars.

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

    https://people.ast.cam.ac.uk/~wyatt/jw12.pdf
    19 Jun 2012: Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed 18 June 2012 (MN LATEX style file v2.2). Debris from terrestrial planet formation: the Moon-forming collision. Alan P. Jackson1? and Mark C. Wyatt1?1Institute of Astronomy, University of Cambridge,

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