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8 Jul 2009: Thedisc is observed to be larger than the radius of 20 au inferred fora black-body SED (Zuckerman & Song 2004), suggesting some. ... excess is predicted to increase only slightly dur-ing such events and the dusty episode would last 20 Myr (Boothet al.

30 Mar 2009: nm. Using a special interference filter centred on 975.5 nm with a bandwidth of 20 nm, they could search between hydroxyl lines for so-called Lyman-α radiation.

3 Sep 2009: 0.01. 0.1. 1. 10. 5 10 15 20 25 30 35 40 45 50. ... Mou. ter /. ME. arth. Simulation Time. No BinaryBinary, a=20 AU, e=0.5.

12 Feb 2009: tcol = r1.5 M-0.5 (ρrdrDmax/Mtot) (12q-20)(18-9q)-1[11.25(e/I)2]-0.5/G(q,Xc). This can be solved to give:. ... Emission efficiency Qem=Qabs 1 for λ<D and (λ/D)n for λ>D (although there are emission features, e.g., 10 and 20 µm features of silicates

21 Jul 2009: For a statistical analysis, we combine these datawith our prior SCUBA and MAMBO-2 observations of 20 other M-dwarfs. ... This correction amounted to between 5% and 20%of the integrated flux density.

28 Jan 2009: The planets: van de Kamp (1982) proposed 2 planets of 0.5 and 0.7MJ in orbits of 12 and 20 years.

19 Jun 2009: have gas giants (planets with masses equal to orgreater than Saturn) within 20 AU which Marcy et al. ... LHBs is<12% (assuming that Saturn mass planets within 20 AUare required for an LHB).

23 Jun 2009: B 44.2 34.3 1.20 73840 Cal42.2 26.8 0.65 116870 Cal46.1 39.2 0.75 η Corvi Sci46.6 42.4 1.15 107218 Cal. ... 13.7 12.5 10 6.7Wavelength, um. 010. 20. 30. 40. Pix. el.

15 Sep 2009: sample (20 stars total) only weak constraints could be derived. Similarly, a submillimeter.

25 Oct 2009: S2d = 0.54e5/3(1 e2)4/3. (20). 2.4.3 Where do collisions occur, and at what velocity? ... have used the in-clination distribution function given by equation 2.20 of Krivov etal.