... But over this small range in r (the distance to the centre of the Earth), you can use a simpler approximate form of the potential energy equation: PE = mgh Tuesday, 22 February 2011 Where h is the height, m the mass of the ball, and g = 9.8 m s-2. ...
46. http://www.mso.anu.edu.au/~kcf/pubs_top20/103.pdf
... 1 R. P. Kirshner,1 P. Challis,1 J. Tonry,2 R. L. Gilliland,3 R. C. Smith,4 A. Clocchiatti,5 A. Diercks,6 A. V Filippenko,7 M. Hamuy,8 C. J. Hogan,6 B. Leibundgut,9 M. M. Phillips,5 D. Reiss,6 A. G. Riess,7 B. P. Schmidt,10 R. A. Schommer,5 J. Spyromilio,9 ...
47. http://www.mso.anu.edu.au/seminars/abstracts/20150305-1100.html
... The first natural guide star (NGS) and laser guide star (LGS) adaptive optics (AO) systems on 8 to 10 m class telescopes were implemented on the Keck II telescope in 1999 and 2004, respectively. ...
48. http://www.mso.anu.edu.au/~charley/papers/LineweaverGrether03color.ps
... and 8.5 years lie below the curve, due to the lower average sensitivity & 10 m/s of ... 1:8 0:3 0:3 +0:3 0:4 { { Marcy, Butler, Fischer & Vogt 2003 0:7 m { { { Lineweaver ... 2002 0.25-15 M Jup 0-8 yrs (< 4 AU) 6% 9 3% 18 +19 7 % Armitage et al. ...
49. http://www.mso.anu.edu.au/~akarakas/download/Renda_etal2004.pdf
... We adopted the metallicity-dependent yields of Renzini & Voli (1981) for single stars in the mass range 1 - 8 M . ... of 15 kp c. M 1 c 2004 RAS, MNRAS 000, 16 4 A. Renda et al. 1 a 0 -1 -2 -3 10 20 30 40 0 -1 5 -2 -3 -6 -4 -2 0 9 8.5 8 b 2 1 0 ...
50. http://www.mso.anu.edu.au/pfrancis/papers/2126-158.ps
... M i # z # RA # Dec ## # Comments [mag] [mag] [arcsec] [arcsec] [arcsec] [kpc] 35 22.46 21.33 0.8335 42.1 136.7 143.0 1090.7 ... 2004, AJ, 127, 1305 c # 0000 RAS, MNRAS 000, 000--000 8 M. T. Whiting et al Figure 5. ...