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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. arX iv:1 302. 3615 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/vmbw13.pdf
    12 Apr 2013: 100 AU. 200 AU. 500 AU. 1000 AU. Figure 6. The number of orbits taken by an isolated planet arounda star throughout its MS phase.

  3. arX iv:1 310. 1395 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/vewt13.pdf
    8 Oct 2013: 10. 20. 50. 100. 200. Rkpc. UHk. msL. UHRL u sed fo r flyby co m pu tatio n s.

  4. arX iv:1 311. 2947 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/bkwj13.pdf
    14 Nov 2013: ity. 0. 6. 12. 18. 24. 30. 36. 20 200. 30.0Blackbody radius (AU).

  5. arX iv:1 311. 2977 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/mksb13.pdf
    14 Nov 2013: Observations at wavelengths> 200 µm are sensitive to dust that is large enough totrace the planetesimal distribution.

  6. Cambridge STARS Homepage

    https://people.ast.cam.ac.uk/~stars/
    28 Feb 2013: In most circumstances, just 200 points are sufficient. Simultaneous solution of structure and composition.

  7. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130227.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130227.txt
    29 Mar 2013: For the record these are: 20121013 runs 200-205; 20121025 runs 130-139; 20121112 runs 155-168 = not exactly a massive haul!

  8. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130431.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130431.txt
    28 May 2013: For the record, previous (re)processed nights were for missing Chilean data 20121013 200-205 20121025 130-139 20121112 155-168 ] We also spotted since the beginning of P91 that ESO

  9. mnr_15360

    https://people.ast.cam.ac.uk/~wyatt/mw09.pdf
    17 Apr 2013: At this radius, the time-scale for planet stir-ring is only 0.65 Myr, orders of magnitude less than the star’s age(200 Myr; Barrado y Navascues et al.

  10. MNRAS 433, 2334–2356 (2013) doi:10.1093/mnras/stt900Advance Access…

    https://people.ast.cam.ac.uk/~wyatt/kw13.pdf
    16 Jul 2013: 88692 HD 165439 1.2 200 A2 11 Myr? Age uncertain? (22)89046 HD 166191 45.9? ... Inany case, removal of the coolest few sources (those below 200 Ksay) would make little difference to our analysis.

  11. Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pwk13.pdf
    29 Oct 2013: 2010). Possible (< 3σ) detection of orbital motionη Tel-B 48 2 200 6 Neuhäuser et al.

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