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19 Apr 2006: They used this result to explain the inner hole in the  Pictoris disk by a planet at 20 AU:. ... 850 m : 320 m – 20 cm. Since the size cut-off for resonance is 300 m – 2 mm, I predict:.

19 Apr 2006: than 20 per cent for stars with twice the metal content of theSun (Fischer & Valenti 2005; Santos et al. ... HD 13445 (K1V) 0.20 HD 10700 (G8V) 0.36HD 143761 (G0V) 0.14 HD 196378 (F7V) 0.32HD 192263 (K2V) 0.07 HD 20794 (G8V) 0.23HD 117176 (G5V)

19 Apr 2006: Large-scale mapping of the central 5 pc of the Galaxy at10, 20, and 30 lm at 400 angular resolution by Telesco et al.(1996) found a temperature gradient consistent with ... We estimate a uni-form ISM across our 11.7 and 18.2 lm passbands of 2.86and 2.20,

5 Oct 2006: whole southern celestial hemisphere (20,000deg2) to a depth 4 magnitudes fainterthan 2MASS/DENIS in at least two wavebands J and K.

19 Apr 2006: Dominik,5 and H. J. Walker6. Received 2004 September 17; accepted 2004 December 20; published 2005 January 10. ... The total dust flux within a diameter circle is′1 37.0mJy at 850mm and mJy at 450mm, in good2.5 250 20.

19 Apr 2006: The diameter of theP.A. = 1757 5 107major axis of the emission at 10.8 mm is 20.2, which corre-sponds to 215 AU. ... At 18.2 mm the maximum extent of theemission is 20.0 (198 AU), which is about 90% the size ofthe 10 mm emission.

27 Jun 2006: The resulting distance moduli are: dmag = [18.2, 20.9, 16.8] In principle, from the CMD matching, you can't really shift the ridgeline by more than 0.05 mag

17 Jan 2006: A reasonable estimate to account for this is that the 2x2 plots need to be adjusted by 20% (ie. ... However, one of the frames exhibited a large magnitude term in y amounting to 0.05 pixel (20 mas) over the observed magnitude range.

19 Apr 2006: wing along lines through the star. The nine evenly spaced contour levels are at the 10, 20,. ... We ignore results for the regionwithin 20 AU of the star because of the contribution of the silicate feature and uncertaintiesin the PSF.

26 Jan 2006: The images mimic fuzzy looking galaxies and in this image peak at typically 5-20 counts above sky. ... measured using a conventional method) is therefore also 1.20 (Parseval's Theorem and power spectrum <-- FT --> autocorrelation).