Search
Search Funnelback University
- Refined by:
- Date: 2018
21 -
30 of
42
search results for TALK:PC53 20 |u:people.ast.cam.ac.uk
where 0
match all words and 42
match some words.
Results that match 1 of 2 words
-
M. Pettini: Introduction to Cosmology — Lecture 1 BASIC ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture01.pdf8 Oct 2018: 20 0 20. 0. 0.5. 1. NowBBNEWPlanck. Figure 1.9: Λ as a function of the scale factor a, for a universe in which m,0 = 0.3and Λ,0 = -
Draft version January 1, 2018Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/mwoa18.pdf2 Jan 2018: 2). 6 Matrà et al. 20 10 0 10 20v-v (km/s). ... 20 10 0 10 20v-v (km/s). 8. 6. 4. 2. 0. -
M. Pettini: Introduction to Cosmology — Lecture 9 RECOMBINATION ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture09.pdf6 Nov 2018: c dt. a(t). (9.20). We want shor at redshift z. Using ȧ = da/dt, dt = da/ȧ = da/aH, wehave:. -
Mon. Not. R. Astron. Soc. 000, 1–23 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/kmwk18.pdf22 Nov 2018: 5.00. 4.75. 4.50. 4.25. 4.00. log(Σ0). 20 30 40 50. T0. ... 5.0. 4.5. 4.0. log(Σ0). 20 25 30 35 40. T0. 0.0. -
Introduction to CosmologyLecture 10 R K Sachs A M ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture10_slides.pdf6 Nov 2018: Kunz. 20,70,3, H. Kurki-Suonio. 30,52, G. Lagache. 5,70, A. Lähteenmäki. 2,52, J.-M. -
Analysis of the Herschel DEBRIS Sun-like star sample
https://people.ast.cam.ac.uk/~wyatt/skwl18.pdf19 Feb 2018: 3040. N. 0 10 20 30 40N. F spectral typeG spectral typeK spectral typeDUNES target. ... 20. 30. 40. 50. 60. 70. Num. ber. F spectral typeG spectral typeK spectral type. -
M. Pettini: Introduction to Cosmology — Lecture 8 PRIMORDIAL ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture08.pdf30 Oct 2018: n. p= exp. [mc. 2. kTd. ]= exp. [1.3. 0.8. ]= 0.20 = 1 : 5 (8.6). ... 0.43. 20. Figure 8.4: The abundances of light elements relative to H predicted by BBN calculationsare shown as functions of η nb/nγ (bottom x-axis) and b,0h2 -
M. Pettini: Introduction to Cosmology — Lecture 13 COSMOLOGICAL ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture13.pdf14 Nov 2018: By z = 0, the intensity of the UV background has decreased by a factorof 20. -
MNRAS 000, 1–23 (0000) Preprint 6 June 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mbwk18.pdf31 Jul 2018: MNRAS 000, 1–23 (0000). 4. 0 20 40 60 80 100Semi-major axis [AU]. ... Lower right panel: chains of equal mass planets withK0 =12, 20 and 30. -
M. Pettini: Introduction to Cosmology — Lecture 10 FLUCTUATIONS ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture10.pdf6 Nov 2018: δT. T. )SW. =1. 3. δΦ. c2. (10.20). There are two competing effects here. ... 10.20. Note that there is no scale dependence of the temperature fluctuations ineq.
Search history
Recently clicked results
Recently clicked results
Your click history is empty.
Recent searches
Recent searches
Your search history is empty.