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11 - 20 of 31 search results for KaKaoTalk:ZA31 24 24 |u:people.ast.cam.ac.uk where 0 match all words and 31 match some words.

  1. Results that match 2 of 3 words

  2. arX iv:1 803. 1126 5v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/edhm18.pdf
    2 Apr 2018: 95418 β UMa 4 A1 IV 2.341 2.38 4.2 24.5 316 Y/N 5,6. ... 173667 110 Her 0.126 0.096 0.101 0.115 24 0.561 0.157 cons.

  3. M. Pettini: Introduction to Cosmology — Lecture 2 NEWTONIAN ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture02.pdf
    10 Oct 2018: ρ 1a4. (2.23). 7. and. a(t) =. (t. t0. )1/2; ρ(t) =. ρ0a4. =ρ0t. 20. t2(2.24). This is the second classic cosmological solution.

  4. Noname manuscript No.(will be inserted by the editor) Space-based ...

    https://people.ast.cam.ac.uk/~wyatt/dlab18.pdf
    31 Jul 2018: radius, and albedo Cont. 3 8.16 9.24 8.67 83 Existence of atmosphere Cont. ... The Messenger 143:16–24. Errmann R, Minardi S, Labadie L, Muthusubramanian B, Dreisow F, NolteS, Pertsch T (2015) Interferometric nulling of four channels with

  5. M. Pettini: Introduction to Cosmology — Lecture 5 REDSHIFTS ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture05.pdf
    18 Oct 2018: 2.21 and 2.24). Thus,we do have a horizon. We also recall (from eq. ... 2.24). With this func-tional form, we find that in the radiation dominated era, the horizon scalewas.

  6. MNRAS 000, 1–11 (2015) Preprint 9 November 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/khhw18.pdf
    9 Nov 2018: θ λ Depth. 3542116 1268.2 11.0 1.05 0.24 0.23 0.001033542116 991.9 8.3 1.08 0.28 0.25 0.00074. ... For KIC 8027456, assuming M? = 2M, R? = 1.5R?,and θ = 0.24 days yields an upper limit of rt < 1.4au, and acircular period of 1.1 years.

  7. M. Pettini: Introduction to Cosmology — Lecture 6 THE ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture06.pdf
    23 Oct 2018: 9. 14. 16. 18. 20. 22. 24. 0.0 0.2 0.4 0.6 0.8 1.01.0. ... ρk = 3. 8πG. k. a2(6.24). which varies as ρk a2, so that for curvature w = 1/3.

  8. Introduction to CosmologyLecture 10 R K Sachs A M ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture10_slides.pdf
    6 Nov 2018: Savelainen. 30,52, G. Savini. 96. , D. Scott. 24. , M.

  9. Debris Disks: Probing Planet Formation Mark C. Wyatt Abstract ...

    https://people.ast.cam.ac.uk/~wyatt/wyat18.pdf
    20 Jul 2018: 2015);e.g., stars in such regions that do not show evidence of 24 µ m emission above pho-tospheric levels are designated as class III stars (as opposed to class ... I or II starsfor which excess 24 µ m emission is present), and are normally considered

  10. M. Pettini: Introduction to Cosmology — Lecture 1 BASIC ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture01.pdf
    8 Oct 2018: In cgs units:. H0 = 3.24 1018h s1 (1.11). Clearly, the time for a galaxy at a distance d, moving at velocity v, to moveapart by a further distance d

  11. Mon. Not. R. Astron. Soc. 000, 1–23 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/kmwk18.pdf
    22 Nov 2018: 8715. 16. 80 88 96 104. R0. 0.06. 0.12. 0.18. 0.24. ... 0.06. 0.12. 0.18. 0.24. h. h = 0. 160. 060. 09.

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