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21 - 30 of 30 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 30 match some words.

  1. Results that match 1 of 2 words

  2. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/smw15.pdf
    15 Jan 2015: 140. 160. 180. 200. 220. 240. 260. 0 105 2x10. 5 3x10. ... 5. Angle. Time (yrs). 100. 120. 140. 160. 180. 200. 220.

  3. Next Generation Very Large Array Memo No. 6Science Working ...

    https://people.ast.cam.ac.uk/~wyatt/ihmg15.pdf
    24 Oct 2015: The region inside the first gap is optically thick (T > 200 K); additionalouter rings may be optically thick as well. ... These objects (see Figure 2) arepresumably in the latest phase of accretion in the formation of stars moremassive than 10 or 20 M

  4. arX iv:1 501. 0414 4v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dhsk15.pdf
    20 Jan 2015: 11 –. 0 100 200 300 400 500 600 700Photometric aperture radius [mas].

  5. MNRAS 000, 1–14 (2015) Preprint 17 December 2015 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/rw15.pdf
    17 Dec 2015: MNRAS 000, 1–14 (2015) Preprint 17 December 2015 Compiled using MNRAS LATEX style file v3.0. Dynamical Constraints on Outer Planets in Super-Earth Systems. Matthew J. Read1? and Mark C. Wyatt11Institute of Astronomy, University of Cambridge,

  6. https://people.ast.cam.ac.uk/~optics/dazle/sky-data/Rousellot_list_v2.…

    https://people.ast.cam.ac.uk/~optics/dazle/sky-data/Rousellot_list_v2.0.dat
    16 Jun 2015: 1.758e-08 8141.200 2.949e-01 8141.502 2.949e-01 8141.831 7.771e-03 8142.440 7.771e-03 8144.889 2.110e-07 8145.328 ... 294 4.656e01 9444.336 1.324e-01 9444.342 1.324e-01 9444.858 2.932e-04 9445.978 2.932e-04 9449.923 9.369e-01 9450.200

  7. arX iv:1 501. 0318 1v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/asgw15.pdf
    15 Jan 2015: unfiltered STIS observations (200-1,050 Å) and the filtered F606W ACS images. ... 24 –. Disk Spine Position: Observations and Models. -200 -100 0 100 200Distance [au].

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

    https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf
    25 Nov 2015: arX. iv:1. 511. 0591. 9v1. [ast. ro-p. h.E. P]. 18 N. ov 2. 015. Mon. Not. R. Astron. Soc.000, 1–18 (2002) Printed 19 November 2015 (MN LATEX style file v2.2). IR-excesses around nearby Lambda Boo stars are caused by debrisdisks rather than ISM

  9. Accepted to ApJ: October 28, 2015Preprint typeset using LATEX ...

    https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf
    2 Nov 2015: Some young (10–200 Myr)debris disks have also shown mid-IR variability on similarscales, interpreted as debris from planetesimal collisions(e.g., Melis et al.

  10. /astro/p7scch2/AUMic/paper/figures/all.eps

    https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf
    16 Jun 2015: m1,e1,p1 4.2M3 1.5 103 100 0.05. M4 1.4 103 200 0.05.

  11. Draft version January 19, 2015Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/mmks15.pdf
    19 Jan 2015: 0.090.14. 7 7 2/10 0.200.070.17 3/11 0.27. 0.090.16. 8 1y 7/48 0.150.040.07 7/48 0.15. ... 0.100.15. 19 7o 2/10 0.200.070.17 3/11 0.27. 0.090.16. a Unconfirmed planetary systems are HD 22049 ( Eri), HD 10700 (τ Cet) andHD

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