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    21. http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight.ps
    ... red multi­object spectrograph on an 8­m class telescope (or preferably several of ... Every one of you gets more 8­m class telescope time than the whole of Australia ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight.ps -- 153.9 Кб -- 30.08.1998
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    22. http://www.mso.anu.edu.au/~geoff/HEA/11_Accretion_Disks_II.pdf
    ... supermassive black hole in an AGN are M a = 0.1 M O /yr and M = 10 8 M O giving: L 4.7 в10 37 W (2.1-6) r0 1 / 2 1 / 4 5 r ­3 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/11_Accretion_Disks_II.pdf -- 813.5 Кб -- 12.06.2003
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    23. http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L16/gyro2.py
    ... rate of change of azimuthal angle ## Comment in the following statements to get pure precession #if abs(cos(theta)) < 1e-8: # phidot = M*g*r/(I*alphadot) #else: # phidot = (-alphadot+sqrt(alphadot**2+2*M*g*r*cos(theta)/I))/cos(theta) pedestal = box(pos ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L16/gyro2.py -- 4.1 Кб -- 29.03.2011
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    24. Gemini Near-Infrared Integral-Field Spectrograph (NIFS) Diffraction.
    ... The diffraction image FWHM at 2.2 microns on the Gemini 8 m telescope is about 0.07". ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/nifs/description/diffraction.shtml -- 5.3 Кб -- 02.10.2012
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    25. http://www.mso.anu.edu.au/~geoff/AGD/Winds.pdf
    ... 0.62 6 G = 6.67 10 ­ 27 ­ 11 SI 8 (16) m = 1.66 10 T = 1.5 10 K 8 kg Solar radius = 6.96 10 m ­ 3 = 1.55 1014 m ­ 3 Electron ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/AGD/Winds.pdf -- 918.1 Кб -- 03.03.2016
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    26. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Rautiainen04
    ... For our analysis, we used even components m = 0-8. ... with a dotted line, m = 6 with a dashed line and m = 8 with a dot-dashed line ... The m = 6 and m = 8 components also have two maxima, the inner coinciding with the m ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Rautiainen04 -- 1663.8 Кб -- 09.07.2007
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    27. http://www.mso.anu.edu.au/~geoff/AGD/Instabilities.pdf
    ... for there to be no instability is: v cos m = ------------------ 8 c1 Astrophysical Gas Dynamics: Kelvin-Helholtz Instability ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/AGD/Instabilities.pdf -- 225.5 Кб -- 19.08.2012
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    28. http://www.mso.anu.edu.au/~charley/papers/Dopita2011.pdf
    ... 1052 ionizing photons s-1 for a halo mass of log M/M = 11, and as many as 8 в 1054 ionizing photons s-1 for a halo mass of log ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/Dopita2011.pdf -- 414.2 Кб -- 19.10.2011
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    29. Research Interests
    ... You are the best, and you know it. Every one of you gets more 8-m class telescope time than the whole of Australia combined. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node12.html -- 5.6 Кб -- 02.10.2012
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    30. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Conselice05
    ... more massive than, and less massive than, the average halo mass, Mhalo = 1011.8 M ... the most extreme cases occurring in ob jects with halo masses Mvir > 1011.8 M ... The higher average M /Mvir value at z > 0.8 is likely produced by our selection of ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Conselice05 -- 240.6 Кб -- 19.12.2006
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