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21 - 30 of 35 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 35 match some words.

  1. Results that match 1 of 2 words

  2. MNRAS 000, 1–19 (2019) Preprint 20 December 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/aght19.pdf
    17 Jan 2020: MNRAS 000, 1–19 (2019) Preprint 20 December 2019 Compiled using MNRAS LATEX style file v3.0. ... MNRAS 000, 1–19 (2019). Dipper Disc Inclinations 11. 0.00.20.40.60.81.0cos(id). 0. 2.

  3. M. Pettini: Introduction to Cosmology — Lecture 15 CLUSTERS ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture15.pdf
    28 Jun 2020: 3=. [1. 4. (6π. t. tmax. )2/3]3=. (6π)2. 43= 5.55 (15.20). ... 15.20) to 5.55 8 4, or. 1 δvirnonlin ' 178 (15.22).

  4. MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/kw20.pdf
    18 Aug 2020: 20). Mmindisc is the total disc mass up to that size skm (Eq. ... Figure 6b confirms this, albeit at a low. MNRAS 000, 1–20 (2020).

  5. MNRAS 000, 1–11 (2020) Preprint 26November 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/zcac20.pdf
    26 Nov 2020: stellar companions with separations> 20 au mostly affect discs inthe upper 10% of the discmass and size distributions. ... The frequencyof visual companion multiplicity in Lupus in the range 20-4800au is then 12% (13/105).

  6. MNRAS 000, 1–7 (2019) Preprint 28 January 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mwkk19.pdf
    28 Jan 2020: P] 2. 7 Ja. n 20. 20. 2 S. Marino et al. ... The grey. contours show emission above 5, 10 and 20 times the rms level.

  7. The Dynamics of Scarlet Fever Epidemics in England and Wales in the…

    https://people.ast.cam.ac.uk/~vasily/data/scarlet.pdf
    18 Oct 2020: was the only one that was reliably identified in the 19th century [20]. ... Phil Trans R Soc Lond B 1995; 348: 309-20. 3. Anderson RM, May RM.

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

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture12.pdf
    17 Nov 2020: In. <0.8, 2!3, >20. 0.8!1, 3!5. 1!1.5, 5!10. 1.5!2, 10!20. 0.8. ... 1. 1.5. 2. 3. 5. 10. 20. 3.54.04.5!2. 0. 2. 4.

  9. MNRAS 000, 1–14 (2020) Preprint 8October 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/xkwy20.pdf
    8 Oct 2020: 2013),whileprojected rotation speedsare foundbe to 𝑣 sin 𝐼 = 3.20.5kms1(Henry et al. ... 2007b)find that theplanetesimals canbe stably located between 0.4 0.8,20 50, or beyond 60 au.

  10. Draft version June 29, 2020Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mdwm20.pdf
    29 Jun 2020: a synthesized beam of 1.8′′ 0.9′′ with a position angle(PA) of -20.8. ... tenna illumination patterns only out to the 20% power. level3; therefore, we focus on our results within 33.4′′. (

  11. Mon. Not. R. Astron. Soc. 000, 1–21 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/kmkm20.pdf
    8 Jul 2020: the Keplerian velocity at 20 au which is equal to 8.4 km/s(i.e. ... 20 25 30 35. i. 100 0. 100. PA. 9.6. 9.9.

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