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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.

  1. Results that match 1 of 2 words

  2. 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.

  3. 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

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

    https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf
    2 Nov 2015: EPIC 203410665 (V V896 Sco) and 203937317(DoAr 24) are both well-known members of ρ Oph thathave been studied in the near-IR (e.g., Furlan et al. ... 204630363 407050 K7.5 0.810.130.13 24.2118.2 — — — 15 C F/(P)TD.

  5. 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.

  6. Draft version May 29, 2015Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/cwmm15.pdf
    14 Sep 2015: Draft version May 29, 2015Preprint typeset using LATEX style emulateapj v. 5/2/11. A COMPACT CONCENTRATION OF LARGE GRAINS IN THE HD 142527 PROTOPLANETARY DUST TRAP. Simon Casassus1,2, Chris Wright3, Sebastian Marino1,2, Sarah T. Maddison4, Al

  7. 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

  8. https://people.ast.cam.ac.uk/~optics/cirsi/ociw/g133_dupont.tcs

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/g133_dupont.tcs
    16 Jun 2015: position! G133_NW_D 01 03 42.43 -06 34 24.2 J2000.0 G133_NW_A 01 03 29.57 -06 34 24.2 J2000.0 G133_NW_C 01 ... G133_NE_D 01 04 30.43 -06 34 24.2 J2000.0 G133_NE_A 01 04 17.57 -06 34 24.2 J2000.0 G133_NE_C 01 04

  9. The LCIR survey at Cambridge

    https://people.ast.cam.ac.uk/~optics/cirsi/lcirs/
    16 Jun 2015: Wavebands and limiting magnitudes. band Nominal limiting mag 5sigma is 1.5 diameter aperture U from WHT [24.5] B from WHT [25.5] V from CTIO BTC 26.5 R ... SSA22 22 17 54.0 00 14 34. NICMOS 22hr 22 20 17.2 -24 43 27.

  10. CIRPASS

    https://people.ast.cam.ac.uk/~optics/cirpass/proposing.html
    16 Jun 2015: Last modified: Wed Nov 24 12:12:42 1999.

  11. https://people.ast.cam.ac.uk/~optics/cirsi/ociw/xmm-lbqs2215_dupont.tc…

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/xmm-lbqs2215_dupont.tcs
    16 Jun 2015: position XMM-LBQS2215-C_D | 22:15:38.71 | -17:42:24.2 | 2000 | 0 | XMM-LBQS2215-C_A | 22:15:25.29 | -17:42:24.2 | 2000 | 0 | ... 15:32.00 | -17:44:00.0 | 2000 | 0 | XMM-LBQS2215-NW_D | 22:15:13.70 | -17:36:24.2 | 2000 | 0 | XMM-LBQS2215-NW_A |

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