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1 - 10 of 77 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 77 match some words.

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

    https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf
    16 Jun 2015: arX. iv:1. 506. 0456. 4v1. [ast. ro-p. h.E. P]. 15 J. un 2. 015. Astronomy & Astrophysicsmanuscript no. AUMic c ESO 2015June 16, 2015. Collisional modelling of the AU Microscopii debris discCh. Schüppler1, T. Löhne1, A. V. Krivov 1, S. Ertel2,

  3. arX iv:1 501. 0131 9v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/wbkr15.pdf
    8 Jan 2015: K2.5V 0.072 1.30 n (T08)9826 υ And 01:36:47.84 41:24:19.6 3.5 F9V 0.136 2.36 n (A13) n ... 55.84 -09:27:29.7 3.2 K2V 0.172 7.39 n (A13) y (B09)22484 LHS 1569 03:36:52.38 00:24:06.0 14.0 F8V

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

    https://people.ast.cam.ac.uk/~wyatt/smw15.pdf
    15 Jan 2015: δE Gm (1 β)2ap. (1 2) , (24). and equating the two energies yields. ... 3. Allow-ing for capture into lower j resonances, the overall captureprobability into the 6:5 mean motion resonance for particleswith similar initial conditions is 0.24.

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

    https://people.ast.cam.ac.uk/~wyatt/rw15.pdf
    17 Dec 2015: T =2. πb(2)3/2(α). (a2a1. )5/2  f 2(1 L2. L1. )24.

  6. Mon. Not. R. Astron. Soc. 000, 1–14 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pw15.pdf
    14 Sep 2015: Mon. Not. R. Astron. Soc. 000, 1–14 (2002) Printed 17 July 2015 (MN LaTEX style file v2.2). Double-ringed debris discs could be the work ofeccentric planets: explaining the strange morphology ofHD 107146. Tim D. Pearce? and Mark C. WyattInstitute

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

    https://people.ast.cam.ac.uk/~wyatt/mmks15.pdf
    19 Jan 2015: 1 1 29/204 0.140.020.03 29/204 0.14. 0.020.03. 2 2 24/182 0.130.020.03 22/179 0.12. ... 6 1o 21/146 0.140.020.03 8/33 0.24. 0.060.09 7/49 0.14. 0.040.06 6/64 0.09.

  8. arX iv:1 412. 0675 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwbb14.pdf
    15 Jan 2015: arX. iv:1. 412. 0675. v1 [. astr. o-ph. EP. ] 1. Dec. 201. 4DRAF T VERS IONDECEMBER 3, 2014Preprint typeset using LATEX style emulateapj v. 5/2/11. EXO-ZODI MODELLING FOR THE LARGE BINOCULAR TELESCOPE INTERFEROMETER. GRANT M. K ENNEDY1, M ARK C.

  9. arX iv:1 503. 0207 3v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf
    10 Mar 2015: Theco-added spectrum consists of 27 observations of 20 minutesduration each, over 5 nights between 12 Nov 2013 and 24 Dec2013. ... albe. do. Qabs (24)Qsca (H)Qabs (H)Albedo. Figure 10. Scattering and absorption properties for silicate/organicgrains as a

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

    https://people.ast.cam.ac.uk/~wyatt/ihmg15.pdf
    24 Oct 2015: 24. 5 Chemical evolution of the star and planet forming environ-ment 275.1 Complex organic molecules in Hot Molecular Cores. ... The cyan contours are –6, –3, 3, 6, 12, 24, 48, 96, 192 σI, whereσI = 19.5µJy bm1 is the rms noise in the Stokes I map.

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

    https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf
    25 Nov 2015: 110411† 154 7.0‡ 67.3 7.0‡. 125162 272 15‡ 142 12‡. 183324† 25.4 1.1 17.2 3.3198160 30.7 1.2 14.3 1.7221756† ... Star (HD) µra(mas/yr) µdec(mas/yr) vrad(km/s) Parallax(′′ ) Distance (pc). 11413 -48.27 0.24 -4.42 0.30 3.0 0.7 12.96

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