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1 - 21 of 21 search results for katalk:PC53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 21 match some words.

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  2. Media Activity for Carolin Crawford in 2017 In our ...

    https://people.ast.cam.ac.uk/~csc/newcv/2017media.html
    24 Jul 2019: 24 Mar. Studio discussion about the Cambridge Science Festival. BBC Radio Cambs.

  3. A planet-forming circumbinary disc in a polar configura-tion Grant ...

    https://people.ast.cam.ac.uk/~wyatt/kmfm19.pdf
    17 Jan 2019: 16.5. 18.0 88 80 72 64 24. 625. 225. 826. 427. ... y0. 12 16 20 24 24.0. 25.5. 27.0. 28.5. i. 0.24.

  4. Media activities for Carolin Crawford in 2008 Home Planet ...

    https://people.ast.cam.ac.uk/~csc/newcv/2008media.html
    24 Jul 2019: Brief live phone interview discussing the close approach of the asteroid 2007 TU 24 that morning.

  5. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture15.pdf
    19 Nov 2019: 21. predict, combining eqs. 15.19 and 15.21:. Ṁv. (RR. )1/2 L1/α [M(1 Γ)]3/21/α (15.24). ... 15.24 becomes unimportant, leaving only the term L1/α = L1.5 onthe r.h.s.

  6. Media activity for Carolin Crawford in 2007 BBC Radio ...

    https://people.ast.cam.ac.uk/~csc/newcv/2007media.html
    24 Jul 2019: BBC Radio Cambridgeshire. 24 Sep 2007. Brief live phone interview discussing the Invisible exhibition at the Institute of Astronomy.

  7. Media Activity for Carolin Crawford in 2009 Naked Astronomy ...

    https://people.ast.cam.ac.uk/~csc/newcv/2009media.html
    24 Jul 2019: Home Planet BBC R4. 24 February 2009. Guest panellist. Naked Scientists BBC Radio Cambridgeshire.

  8. 1906.08797

    https://people.ast.cam.ac.uk/~wyatt/smkb19.pdf
    20 Nov 2019: Spitzer/MIPS 24 671 mJy 8Herschel/PACS 70 79424 mJy 9b. Spitzer/MIPS 70 78879 mJy 10Herschel/PACS 100 107167 mJy 9b. ... 2010). flux excess at 24 µm that this model does not accountfor.

  9. Media Activity for Carolin Crawford in 2010 Naked Astronomy ...

    https://people.ast.cam.ac.uk/~csc/newcv/2010media.html
    24 Jul 2019: 25 March 2010. BBC Radio Cambridgeshire. 24 Mar 2010. phone interview discussing the Dark Skies 2010 initiative.

  10. Media Activity for Carolin Crawford in 2013 BBC Radio ...

    https://people.ast.cam.ac.uk/~csc/newcv/2013media.html
    24 Jul 2019: BBC Radio Cambridgeshire. 24 Feb 2013. guest slot on the Mark Rumbold programme discussing asteroids and comets.

  11. A planetesimal orbiting within the debris discaround a white ...

    https://people.ast.cam.ac.uk/~wyatt/mgeh19.pdf
    25 Apr 2019: 24 Institute of Astronomy, Madingley Rd, Cambridge CB3 0HA, UK25 Gemini Observatory, Northern Operations Center, 670 N. ... the disc. (iii) The photoelectric instability (PEI, (24)) can possibly produce arc-shaped struc-.

  12. Educational and Outreach talks for CS Crawford in 2007 ...

    https://people.ast.cam.ac.uk/~csc/newcv/2007talks.html
    24 Jul 2019: June & July. 10,24,24,15. Life in the Solar System. Talk and tour of IoA telescopes to yr 5 pupils from Sancton Wood School, Cambridge.

  13. Educational and Outreach talks and activities for Carolin Crawford ...

    https://people.ast.cam.ac.uk/~csc/newcv/2010talks.html
    24 Jul 2019: May. 24. Big numbers, stars and black holes. Talk to KS2 pupils at St James the Great School, Southwark as part of the Southwark Splash project.

  14. MNRAS 000, 1–21 (2018) Preprint 11 July 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/yksw19.pdf
    11 Jul 2019: For sources not detected at 70 µm,we place an aperture at the 24 µm position to estimatethe flux. ... channel, in some cases only one MIPS 70 µm flux is ex-tracted even if there are two MIPS 24 µm sources nearthe same position.

  15. Draft version April 2, 2019Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/dhcf19.pdf
    3 Apr 2019: Vertical Structure in the AU Mic Debris Disk 3. Observational parameters 2014 Mar 26 2014 Aug 18 2015 Jun 24. ... 330 15 µJy beam1 at a separation of 24.1 0.2 auand PA of 308.2 0.4.

  16. Extrasolar Kuiper Belts Mark C. Wyatt Abstract Extrasolar debris ...

    https://people.ast.cam.ac.uk/~wyatt/wyat19.pdf
    26 Sep 2019: excess emission abovephotospheric levels at different wavelengths (typically at 24, 70, 100 and 160 µ m).Surveys have been carried out for nearby stars with a variety of spectral types, ... Kenyon and Bromley 2010), sincebroad disks are hot early on and

  17. MNRAS 000, 1–12 (2018) Preprint 4 December 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/cmfk19.pdf
    11 Apr 2019: 16 0.816 21.1 4.3 3.5 4.32151 2017-08-09 19:04 0.817 24.1 4.1 8.4 4.0. ... 44 1 S 650LP 724.9 0.641 2080 518.9 8.5 613.3 8.3 803.4 8.4 24.9 0.3.

  18. panstarrs.eps

    https://people.ast.cam.ac.uk/~wyatt/sjw19.pdf
    13 Mar 2019: 23 10. 24 10. 25 10. 26 10. 27. 106 107 108 109.

  19. MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mybf19.pdf
    8 Jan 2019: ACA observations weretaken between 24 October 2016 and 23 March 2017, with atotal time on source of 3.6 h and PWV values ranging from. ... Band 7 - 12m 13, 17, 18 Dec 2016 2.2 16 0.′′55 0.′′48 (73) 46 and 360Band 7 - ACA 24-27 Oct 2016 3.6 175

  20. MNRAS 000, 1–21 (2019) Preprint 23 October 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/wks19.pdf
    23 Oct 2019: MNRAS 000, 1–21 (2019) Preprint 23 October 2019 Compiled using MNRAS LATEX style file v3.0. Susceptibility of planetary atmospheres to mass loss and growth byplanetesimal impacts: the impact shoreline. M. C. Wyatt1?, Q. Kral2, C. A. Sinclair11

  21. Draft version February 13, 2019Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mwwd19.pdf
    14 Feb 2019: Draft version February 13, 2019Typeset using LATEX twocolumn style in AASTeX62. Kuiper Belt-Like Hot and Cold Populations of Planetesimal Inclinations in the β Pictoris Belt Revealed by ALMA. L. Matrà,1, M. C. Wyatt,2 D. J. Wilner,1 W. R. F.

  22. MNRAS 000, 000–000 (2018) Preprint 21 February 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mphp19.pdf
    21 Feb 2019: Assuming C18O traces total disc mass, Q(R) forthis disc reaches a minimum 24 at 80 au confirming thatthe disc is stable against gravitational collapse.

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