Search

14 May 2009: This involved using the One-Mile Radio Telescope of the Mullard Radio Astronomy Observatory to observe a sample of 200 bright radio sources in the 3C revised catalogue, at galactic latitudes

17 Feb 2009: Spiral structure at 200 AU implies planet at 150 AU • Same structure seen in Saturn’s rings (Charnoz et al. ... Numerical integrations of star, migrating planet, 200 planetesimals giving capture probabilities for 3:2 resonance:.

12 Jan 2009: Radius, AU 200 400 600 800. Surf. ace. brig. htne. ss.

8 Jul 2009: e. upto approximately 200 au radius for stars at 12–15 pc distance. ... For five precise (G2 V) solar analogues,the fitted disc radii are 100–200 au (Krivov et al.

21 Jul 2009: Fig. 7. Detection rates of cold debris disks versus stellar masses (stel-lar types) for stars younger than 200 Myr. ... All these stars are less than 200 Myr old. Most of the curvesare upper limits (dashed lines).

27 Jan 2009: 2 term is more important than the 6:4 term or 301:200.

28 Jan 2009: 2007, Irwin et al. 2007). Original estimates for 200 detections/month were overestimate (Horne 2003), but field is evolving rapidly, and now getting large numbers of WASP detections and we can

3 Sep 2009: Sep. 200. 9. Mon. Not. R. Astron. Soc.000, 000–000 (2009) Printed 1 September 2009 (MN LATEX style file v2.2).

25 Oct 2009: Later in the paper we adopt K = 2.1 1014 as a fiducial value corresponding to ρ = 2700 kg m3,Dmax = 2000 km and Q?D = 200 J kg. ... In Table 1 we compare the intrinsic collision proba-bilities we find using the Monte-Carlo approach with 200,000

19 Jun 2009: off in the emission spectrum beyond 200 µm.Here we take Xλ = 1 for λ < 210 µm and Xλ = λ/210for λ 210 µm to be consistent with submillimetre obser-vations ... This is given by:. f(e,I) =. 1.25e2 I2. (14). Here we use the value Q?D = 200 J kg1