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  1. Results that match 1 of 2 words

  2. M. Pettini: Introduction to Cosmology — Lecture 9 RECOMBINATION ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture09.pdf
    6 Nov 2018: a1/2da. (9.24). Performing the simple integration and now changing to redshift, we have:.
  3. M. Pettini: Introduction to Cosmology — Lecture 10 FLUCTUATIONS ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture10.pdf
    6 Nov 2018: IRJνIRJν. = 2y (10.23). and. y =. kT. mec2σT ne dl (10.24). ... Note that the so-called. Compton y parameter in eq. 10.24 increases with T, since the temperaturedetermines the average energy transfer per scattering event.
  4. 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.
  5. M. Pettini: Introduction to Cosmology — Lecture 12 PHYSICAL ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture12.pdf
    13 Nov 2018: 20. 8πGmH(12.16). (Y is the baryonic mass fraction in He: Yp = 0.24) and. ... bT (. 2kT. mH. )1/2= 12.8 T. 1/24 km s. 1 (12.22).
  6. M. Pettini: Introduction to Cosmology — Lecture 16 DARK ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture16.pdf
    22 Nov 2018: 16.22 is: 〈. v2〉. = 3 (880 km s1. )2(16.24). The half-mass radius is trickier. ... Experimentsusing solar, atmospheric, and reactor neutrinos have measured mass dif-. 24.
  7. MNRAS 000, 1–23 (2015) Preprint 30 July 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/bwkk18.pdf
    30 Jul 2018: 24). to eject particles, as for some planets, particles migrate pasttoo fast for them to be ejected. ... 24), and the solid line shows where the timescale for accretion is equal to that for PR-drag, according to the empiricalfit presented here,
  8. 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
  9. 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.
  10. 30 Jul 2018: F7 V 4.126 2.83 2.4 13.7 137 N/– [22, 24, 28]. ... J., Stapelfeldt,K. R., and Wyatt, M. C., “Target Selection for the LBTI Exozodi Key Science Program,” ApJS 216, 24(Feb.
  11. 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.

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