... M 1 2 22 Higgs potential Massive scalar field Self-interacting scalar field (35) (36 ... solved to give == (t) a(t) m mP l = i - t, 12 = ai ex p 4 m 3 mP l (50) m mP l t i t ...
123. http://www.mso.anu.edu.au/pfrancis/comets/comets.pdf
... find that the differential number of comets per unit mass m go es as: dn m-1.04±0.1 ... 46, 205 Bailey, M.E. & Stagg, C.R. 1988, MNRAS, 235, 1 Bailey, M.E., Chambers, J.E ... G.M., Allen, R.L., Brown M.E., Holman, H. & Malhotra, R. 2004, AJ, 128, 1364 ...
124. http://www.mso.anu.edu.au/~bessell/FTP/KS/thar.arc
... XXX Ar, .XXXX Th) * Amended by Gerry Gilmore 17 July 1990 to extend further into UV * (from 2891.2494 to 2993.6311) * Amended by M Bessell November 1990 with additional Ar and Th lines * longwards of 7500 A 2891.2494 ThII 2891.6125 ArII 2891.7301 ThII ...
125. http://www.mso.anu.edu.au/~geoff/HEA/10_Accretion_Disks_I.pdf
... 2, M.S. Longair, Cambridge University Press Active Galactic Nuclei, J.H. Krolik, Princeton Series in Astrophysics High Energy ...
126. http://www.mso.anu.edu.au/~charley/papers/RoblesLineweaverAstroph.pdf
... M ] Age [Gyr] [Fe/H] [C/O] [Mg/Si] v sin i [km s-1 ] e Zmax [kp c] RGal [kp c] Mgal ... inclination (see Sec. 2.5). e Sub-set of stars within the mass range: 0.9 M M 1.1 M ...
127. http://www.mso.anu.edu.au/~kcf/pubs_top20/25.pdf
... M. Wood-Vasey,1 G. Miknaitis,2 C. W. Stubbs,1,3 S. Jha,4,5 A. G. Riess,6,7 P. M ... M., Phillips, M. M., Suntzeff, N. B., Schommer , R. A., Maza , J., & Aviles, R. 1996 ...