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 - 10 of 22 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 22 match some words.

  1. Results that match 1 of 2 words

  2. Observations, Modeling and Theory of Debris Disks Brenda C. ...

    https://people.ast.cam.ac.uk/~wyatt/mkwb14.pdf
    7 Jan 2014: Rhee et al. (2007) havereanalyzed IRAS data and found the detection rate aroundnearby A stars to be 20%. ... 7. 10-24. 10-22. 10-20. 10-18. 10-16. 100. 101. 102. 103. 104.

  3. arX iv:1 312. 5315 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwkd13.pdf
    21 Jan 2014: Dec. 201. 3Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 20 December 2013 (MN LATEX style file v2.2). ... δ offset ("). 20 10 0 -10 -20α cos δ offset ("). -0.06. -0.02.

  4. arX iv:1 312. 4531 v2 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kmlm13.pdf
    21 Jan 2014: 5 Myr. 10 Myr. 20 Myr. E(BV) =0.15. Siess et al. ... 6 G. M. Kennedy et al. 0 10 20 30 40 50θi (deg).

  5. MATHEMATICAL TRIPOS Part III Monday, 11 June, 2012 1:30 ...

    https://people.ast.cam.ac.uk/~wyatt/psd_exam2012.pdf
    23 Jan 2014: MATHEMATICAL TRIPOS Part III. Monday, 11 June, 2012 1:30 pm to 4:30 pm. PAPER 64. PLANETARY SYSTEM DYNAMICS. Attempt no more than THREE questions. There are FOUR questions in total. The questions carry equal weight. STATIONERY REQUIREMENTS SPECIAL

  6. mn.dvi

    https://people.ast.cam.ac.uk/~wyatt/wfpb14.pdf
    23 Jan 2014: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 23 January 2014 (MN LATEX style file v2.2). Stochastic accretion of planetesimals onto white dwarfs:. constraints on the mass distribution of accreted material. from atmospheric pollution. M.

  7. arX iv:1 402. 1184 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/dawk14.pdf
    10 Feb 2014: 15-20% around Main Sequence stars, with increased frequency around younger stars (Su et al. ... function cannot simultaneously match the peak wavelength and the 20–70 µm slope, thus requiring.

  8. Mon. Not. R. Astron. Soc. 000, 1–22 (2013) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/jwbv14.pdf
    11 Mar 2014: 2)moves. From Fig. 2 and the dependencies of Eqs. 16-20 we canalso make some simple general observations about non-sphericallysymmetric distributions of kick angles. ... Figure 2. Distributions of orbital elements for a set of 20,000 particles givena

  9. betapic-final

    https://people.ast.cam.ac.uk/~wyatt/dwra14.pdf
    8 Apr 2014: 755 20. Tielens, A.G.G.M., McKee, C.F., Seab, C.G., Hollenbach, D.J., 1994, ApJ 431, 321 21. ... Contours are 10, 20, 30, 40, 60, 80% of the peak (0.06 Jy/beam).

  10. vpfit9.5.dvi

    https://people.ast.cam.ac.uk/~rfc/vpfit9.5.pdf
    14 Apr 2014: 2. 20. Figure 3: A three component Lyα fit to a region of the sample spectrum,obtained using the methods described in the text. ... log col < (p1) AND log col err > (p2). fixb (p) - added lines have fixed b [20].

  11. Mon. Not. R. Astron. Soc. 000, ??–?? (2014) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/scw14.pdf
    2 Jul 2014: spans of these systems is 20% of the total matching spans ofall systems, and as these simulations are only uncoupled for part oftheir matching span, we conclude that if the scenario ... we proposehere is correct, we are unlikely (< 20%) to find B and C

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.