... m 0 u µ = [ mc, mv i ] = where High Energy Astrophysics: Relativistic Effects 47/92 ... m c ) ) 2 + (67) + m 2 c 2 [ ( d ) 2 + sinh2 ( d 2 + sin2 d 2 ) ] 56/92 (66) High ...
45. http://www.mso.anu.edu.au/~brian/publications.pdf
... Seward, F. D., Schmidt, B., Slane, P., 1995, ApJ, 453, 284 "X-Ray Emission from the Supernova Remnant CTA 1" 106. ... Marcaide, J. M., Alberdi, A., Ros, E., Diamond, P., Schmidt, B., Shapiro, I. I., Baath, L., Davis, R. J., de Bruyn, A. G ...
46. Untitled
... Observatory with Jim Liebert during 1979, showed these stars to be exotic M subdwarfs (paper 58*) and very cool M dwarfs ... star, the bright M subdwarf, had a metallicity of about -0.7 dex while the abundance of VB 12, the faint M subdwarf companion ...
47. http://www.mso.anu.edu.au/~charley/papers/LineweaverDaviesVincent2014.pdf
... PLoS One 8: e65522. 28. Muller M, Mentel M, van Hellemond JJ, Henze K, et al. 2012. ... l v e d t o d i s cr i m in at e i nf ec t i o u s s el f f r o m noninfectious self ...
48. http://www.mso.anu.edu.au/~charley/papers/LineweaverEgan2007.pdf
... m-dis t1ststar s t1stE ar ths tr now tS un ,tE ar th tm- to tlaststar s tpr otondecay tblackholes theatdeath Time after seconds 5.4 в 10-44 [10-43 , 10-33 ] 10-33 -33 , 10-12 ] [10 10-12 [100, 300] 8.9 в 1011 1.2 в 1013 1.2 в 1013 1 в 1016 8 в 1016 1.9 в ...
49. http://www.mso.anu.edu.au/~charley/papers/ChopraLineweaverASSC09v3.pdf
... M icrospor idia Ciliates Animals Plants Fu n g i Fl a g e l l a t e s E u ka r ya ... M: moles per litre; atm: atmosphere] log [Concentration (M)] 5 log [Pressure (atm ...
50. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Seigar06
... M /L) = 1.0, 1.3 and 1.6 (measured in B band solar units), and use our ... M. 1992, ApJS, 81, 413 Mo, H. J., Mao, S., & White, S. D. M. 1998, MNRAS, 295, 319 ... M. F. S., Pastoriza, M. G., Kepler, S. O., & Puerari, I. Ё 1994, A&AS, 108, 41 ...