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21 - 30 of 32 search results for KaKaoTalk:ZA31 24 24 |u:people.ast.cam.ac.uk where 0 match all words and 32 match some words.

  1. Results that match 2 of 3 words

  2. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_09.pdf
    20 Oct 2017: is:. ρεπ 24 rdrdL. =. providing 3rd equation of stellar structure (already have Hydrostatic Equilibrium, and mass conservation from Lecture 6).

  3. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_04.pdf
    13 Oct 2017: Structure & Evolution of Stars 24. Spectroscopic Binaries. 231. 32. 21.

  4. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_02.pdf
    9 Oct 2017: Wien’s Law is extraordinarily useful and worth remembering. Structure & Evolution of Stars 24.

  5. Mon. Not. R. Astron. Soc. 000, 1–27 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/kmwk17.pdf
    5 May 2017: 4 104 100 0.27 1.1 103 40η Tel3 CII 22 48.2 - 24 1.3 102 7.6 104 23HD 219974 CO 14.4 71.9 6 102 60 ... 3 103 1.9 103 10HD 1318357 CO 9.2 122 6 102 50 0.47 1.5 103 16HD 1388136 CO 24.5 150.8 7.4 104 100

  6. Accepted to ApJ: April 6, 2017Preprint typeset using LATEX ...

    https://people.ast.cam.ac.uk/~wyatt/mmkwp17.pdf
    18 May 2017: The total belt flux density determined for the best-fit model is 24.7 0.1 mJy (with an additional 10% uncertaintyfrom flux calibration), consistent with previous flux measurements at slightly ... Foreman-Mackey, D. 2016, The Journal of Open Source.

  7. MNRAS 000, 1–16 (2017) Preprint 21 November 2017 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/xrvv17.pdf
    21 Nov 2017: L. McClain15,22, P. Muirhead13, E. Palle23,24, P. A. Panka12,. J. Provencal25, S. ... 0.16 0.18 0.20 0.22 0.24 0.26 0.28MJD(-57476). 0.0. 0.5. 1.0. 1.5.

  8. Mon. Not. R. Astron. Soc. 000, 000–000 (2017) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/bdjl17.pdf
    5 May 2017: In addition to the main belt seen at long wavelengths,the 24-160 µm spectral energy distribution (SED) fromSpitzer suggests a warmer ring at 20 AU and possibly an-other at

  9. Draft v7.0Preprint typeset using LATEX style AASTeX6 v. 1.0 ...

    https://people.ast.cam.ac.uk/~wyatt/mrdk17.pdf
    11 Sep 2017: KIC 8462852 20 06 15.46 44 27 24.6 11.86 0.54 0.40. ... Star 2 20 06 01.24 44 29 32.4 12.42 0.79 0.51.

  10. arX iv:1 709. 0841 4v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/mcka17.pdf
    26 Sep 2017: HD 138813 A0V 150.8 24.5 US (7) 10 (4) 194/94 9.0 104(2) 1.2 101(3) Y 1.41 0.08(5) 7.5 104.

  11. arX iv:1 701. 0656 8v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/kkpr17.pdf
    5 May 2017: Two other classes are: those occulted by circumstellar material beyond &10au, suchas AA Tau and V409 Tau which show &year-long dimming events [23,24], and systems such as ǫ Aur,

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