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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

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).

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.

23 Jul 2014: and a temperature of57 2K, with the small uncertainty dueto detection over a reasonably wide range of wavelengths (20-160µm). ... Each parameter is calculated at 12 values, giving a gridwith 20,736 models.

4 Dec 2014: 4x109. 6x109. 8x109. 1010. 1.2x1010. 1.4x1010. 0 10 20 30 40 50. ... 107. 108. 109. 5 10 15 20 25 30 35 40 45 50.

31 Jul 2014: 2010) at 100 and160 µm. These data are particularly sensitive to 20 K dust in. ... dark blue respectively. The ALMA sensitivities have been corrected for spatially-resolved emission from dust beyond 11.2 AU (belowroughly 20 K for blackbody grains).

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

13 Oct 2014: Witha binding energy of only 0.754 eV ( 1/20 the binding energy of the electronin neutral hydrogen), corresponding to a wavelength of 16.4 µm, H in animportant source of

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).

4 Dec 2014: 20.614 PsA 7.63 5.76 7.19 0.14 11.0. ... 7Age 450 Myr 43 7 16 6Am 11 2 18 12Ap 5 1 20 18λ Boo 2 2 100.