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1 - 10 of 13 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 13 match some words.

  1. Results that match 1 of 2 words

  2. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_22.pdf
    17 Nov 2017: b) 200 MSun star – generates higher mass elements with CNO greatly reduced as fused into heavier elements.

  3. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf
    10 Nov 2017: Evidence for kinematically distinct outflows – discrete mass-loss episodes (strongly asymmetric)• Expansion velocities 40-50km/s• Kinematic age estimates for features, from distance/velocity, are 200, 400 and 900 years• Smallest

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

    https://people.ast.cam.ac.uk/~wyatt/xrvv17.pdf
    21 Nov 2017: 0.5. 1.0. 1.5. Spitzer:4.5 m. 0 100 200 300 400 500Minutes. ... 1.5. Spitzer:4.5 m. 0 100 200 300 400 500 600Minutes. Nor.

  5. MNRAS 000, 1–14 (0000) Preprint 28 April 2017 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mwkh17.pdf
    5 May 2017: B1 (VLA 1.4 GHz). B2 (Herschel 160-500 µm). -50 0 50 100 150 200. ... For example,when assuming a maximum planetesimal size of 100 and 200 kmin diameter, they found that the optical depth (dominated by thesmallest grains in the disc) stays roughly

  6. Preprint typeset using LATEX style emulateapj v. 01/23/15 DETECTION…

    https://people.ast.cam.ac.uk/~wyatt/mmkwk17.pdf
    18 May 2017: 200 100 0 100 200Distance from star (AU). 200. 100. 0. ... However, the majority of CO emis-. 6 Matrà et al. 60 80 100 120 140 160 180 200 220Semimajor Axis (AU).

  7. arX iv:1 702. 0512 3v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/bfwv17.pdf
    5 May 2017: arX. iv:1. 702. 0512. 3v1. [as. tro-. ph.E. P] 1. 6 Fe. b 20. 17. MNRAS 000, 1–12 (2015) Preprint 20 February 2017 Compiled using MNRAS LATEX style file v3.0. Infrared observations of white dwarfs and the implications. for the accretion of dusty

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

    https://people.ast.cam.ac.uk/~wyatt/bdjl17.pdf
    5 May 2017: Mon. Not. R. Astron. Soc. 000, 000–000 (2017) Printed 5 May 2017 (MN LATEX style file v2.2). The Northern Arc of Eridani’s Debris Ring as Seen byALMA. Mark Booth1,2?, William R. F. Dent3, Andrés Jordán2,4, Jean-François Lestrade5,Antonio

  9. , DRAFT VERSION DECEMBER 23, 2017Typeset using LATEX twocolumn ...

    https://people.ast.cam.ac.uk/~wyatt/baaa18.pdf
    23 Dec 2017: 200, Mountain View, CA 9404356Center of Excellence in Information Systems, Tennessee State University, Nashville, TN 37209, USA57Montsec Astronomical Observatory (OAdM), Institut dÉstudis Espacials de Catalunya (IEEC), Barcelona, Spain58European

  10. Circumstellar discs: What will be next? Quentin Kral, Cathie ...

    https://people.ast.cam.ac.uk/~wyatt/kcw17.pdf
    13 Nov 2017: Circumstellar discs: What will be next? Quentin Kral, Cathie Clarke and Mark Wyatt. Abstract This prospective chapter gives our view on the evolution of the study ofcircumstellar discs within the next 20 years from both observational and

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

    https://people.ast.cam.ac.uk/~wyatt/mrdk17.pdf
    11 Sep 2017: Draft v7.0Preprint typeset using LATEX style AASTeX6 v. 1.0. EXTINCTION AND THE DIMMING OF KIC 8462852. Huan Y. A. Meng1, George Rieke1, Franky Dubois2, Grant Kennedy3, Massimo Marengo4, Michael Siegel5,Kate Su1, Nicolas Trueba4, Mark Wyatt3,

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