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    51. http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L06/Lecture06.pdf
    ... Friday, 4 March 2011 Example · Let's say you do a problem and find that the mg acceleration is given by a= v 1+ c where m is a mass, g is 9.8 m s-2, v is the velocity and c is the speed of light. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L06/Lecture06.pdf -- 885.5 Кб -- 04.03.2011
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    52. http://www.mso.anu.edu.au/~geoff/HEA/mundell.pdf
    ... AJ, 107, 1227 Wilson, A.S. & Ulvestad, J.S., 1983, ApJ, 275, 8 Wrobel, J.M., Patnaik, A.R., Browne, I.W.A & Wilkinson, P.N ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/mundell.pdf -- 623.9 Кб -- 31.05.2000
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    53. http://www.mso.anu.edu.au/~charley/papers/EganLineweaver2008.pdf
    ... 8 G, yet estimates of the dynamic matter density were set at just 30% of that ... 4 K m/s/M pc; that it is flat therefore it is critically dense (tot0 = 2 [8 G/3H0 ... with current cosmological constraints has 8 de m for a significant fraction of ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/EganLineweaver2008.pdf -- 572.1 Кб -- 31.07.2007
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    54. http://www.mso.anu.edu.au/~wood/lectures/2007/assignment_2.pdf
    ... Note. The equation L M 3 is not too bad an approximation for main-sequence stars with M > M : they actually follow a relation L M 3.8 .) ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~wood/lectures/2007/assignment_2.pdf -- 112.4 Кб -- 14.03.2007
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    55. http://www.mso.anu.edu.au/~charley/papers/DavisLineweaverWebb03.pdf
    ... 8 and 9 can be performed numerically by using dt da / a and a 0 , where both are ... 10 The normalized matter density M 8 G 0 /3H 2 and the 0 /3H 2 are constants ... 8 and are plotted in Fig. 3 for the same four models shown in Fig. 2, as well as for ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/DavisLineweaverWebb03.pdf -- 513.7 Кб -- 11.12.2004
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    56. http://www.mso.anu.edu.au/~geoff/HEA/8_Radio_Galaxies.pdf
    ... the size, L , of the emitting region satisfies: 1 day 1 day 13 t ­4 t L < c t = 2.6 в10 ----------- m = 8.4 в10 ----------- pc High Energy Astrophysics: Radio Galaxies 22/56 This estimate will be modified later when we incorporate relativistic effects ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/8_Radio_Galaxies.pdf -- 407.6 Кб -- 27.05.2003
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    57. http://www.mso.anu.edu.au/~nichod/thesis_proposal_dcn.pdf
    ... This is a bright object at a distance of 12.3 Mpc with a neutral hydrogen mass of log(MH I ) = 8.57 M . ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~nichod/thesis_proposal_dcn.pdf -- 889.7 Кб -- 20.11.2009
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    58. http://www.mso.anu.edu.au/annualReport/2003/RSAA_AR2003.pdf
    ... South Adaptive Optics Imager (GSAOI) is being designed and constructed for the Gemini South 8-m diameter telescope in Chile ... Although delayed, NIFS is expected to be commissioned on the Gemini North 8-m diameter telescope in early 2005. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/annualReport/2003/RSAA_AR2003.pdf -- 350.1 Кб -- 03.06.2005
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    59. Answers: Assignment 3
    ... For Planet A, this comes out at 13.5 m s -2 : a little higher than on Earth (9.8 m s -2 ) but probably not uncomfortable. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/MysteryPlanet/Answers_23.htm -- 12.9 Кб -- 17.03.2004
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    60. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Seigar06a
    ... NFW halo with an initial concentration cvir = 12.0 and virial mass 8.7 в 1011 M ... 2000) and the total mass of ^e 8 в 1011 M from kinematics of the Andromeda Stream ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Seigar06a -- 345.6 Кб -- 12.12.2006
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