Search

Search Funnelback University

Search powered by Funnelback
10 results 20 results 50 results
Relevance Date (Newest first) Date (Oldest first) Title (A-Z) Title (Z-A) Distance URL (A-Z) URL (Z-A) Shuffle
1 - 7 of 7 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 7 match some words.

  1. Results that match 1 of 2 words

  2. A Fixed Point in Coptic Chronology: The Solar Eclipse of 10 March, 601

    https://people.ast.cam.ac.uk/~gil/Coptic-Eclipse.pdf
    5 Aug 2011: 190-192]. Zu den Luxusspeisen und -getränken in griechischen Papyri [pp. 193-200].

  3. Astroparticle_15

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_15.pdf
    25 Mar 2011: R is now 200 microns. This is very large on a quantum scale, but small on the scale used to test gravity in experiments – close to current limit of 100

  4. https://people.ast.cam.ac.uk/~vasily/sdss/dropouts/dropouts.txt

    https://people.ast.cam.ac.uk/~vasily/sdss/dropouts/dropouts.txt
    3 Jun 2011: 200.76777495 3.7214707 25.29 24.61 23.14 23.00 19.97 4 140.21862225 30.4611002 23.07 23.08 22.58 20.84 19.00 5

  5. Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/cwds11.pdf
    5 Jul 2011: Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed July 5, 2011 (MN LATEX style file v2.2). Multi-Wavelength Modelling of the β Leo Debris Disc: 1, 2 or 3planetesimal populations? L J Churcher 1†, M.C. Wyatt1, G. Duchêne2,3, B. Sibthorpe4, G.

  6. arX iv:1 104. 0007 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/ramb11.pdf
    5 Apr 2011: Here we assume thatQD = 200 J kg. 1. and that it does not vary withD. ... 0.4. 0.8 200 Myr. Semimajor Axis (AU). Ecc. entr. icity. Log(Water Mass Fraction).

  7. arX iv:1 107. 1239 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/vwmb11.pdf
    16 Nov 2011: HAUL. HAUL. Star. Planet. -350 -300 -250 -200 -150 -100 -50. ... Shown is the eccentricity evolution over 104 years of evolution of a0 = 200 AU planets (orbelt particles; left panel) and a0 = 103 AU planets (or belt particles; right panel) orbiting a

  8. Noname manuscript No.(will be inserted by the editor) DEBRIS ...

    https://people.ast.cam.ac.uk/~wyatt/wcb11.pdf
    28 Mar 2011: Noname manuscript No.(will be inserted by the editor). DEBRIS DISK SIZE DISTRIBUTIONS: STEADY STATECOLLISIONAL EVOLUTION WITH P-R DRAG AND. OTHER LOSS PROCESSES. M. C. WYATT1, C. J. CLARKE1 and M. BOOTH1,2,31 Institute of Astronomy, University of

Refine your results

clear all

Date

Search history

Recently clicked results

Recently clicked results

Your click history is empty.

Recent searches

Recent searches

Your search history is empty.