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    1. http://www.mso.anu.edu.au/~ralph/data/cool/ABOUT.txt
    ... as a function of metallicity are given in the files: mzero.cie : cie cooling for primordial hydrogen/helium mix log(T) = 4-8.5 m-00.cie : cie cooling for solar abundances mix log(T) = 4-8.5 m-05.cie : [Fe/H] = -0.5, solar/primordial average ratios m-10 ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~ralph/data/cool/ABOUT.txt -- 5.5 Кб -- 08.08.2011
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    2. Paul Francis -- Astronomical Constants
    ... Mass of Sun = 1.989 times 10**30 kg . Radius of Sun = 6.96 times 10**8 m . Solar Luminosity = 3.8 times 10**26 W . ... Stefan Boltzmann constant = 5.67 times 10**-8 W m**-2 K**-4 . Square degrees on a sphere = 41253 . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/constants.html -- 2.9 Кб -- 01.10.2012
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    3. http://www.mso.anu.edu.au/~geoff/HEA/Questions%201-8.pdf
    ... 1.24 10 19 1.60 10 --m 34 8 6 --m 1 eV Also, to determine frequency and wavelength given energy, use =h hc = ----1.60 10 ... 3 u (e) For L = 3. 83 10 26 c 4 r2 = L 11 L u = -------------4 cr 2 m = 2.8 10 13 W and r = 1.50 10 u = 4.5 10 6 Jm 3 eV m 3 5 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Questions%201-8.pdf -- 138.6 Кб -- 09.09.2011
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    4. http://www.mso.anu.edu.au/~geoff/HEA/Solns_Q_1-8.pdf
    ... eV ­1 4 m = 1.24 10 ------ eV ­1 ­ 19 ­ 34 8 --- m ­1 eV Angstroms Hence the following table (the primary quantity is given in ... 83 10 26 W and r = 1.50 10 u = 4.5 10 ­6 11 m = 2.8 10 13 Jm ­3 eV m ­3 5. (a) The beam is defined by x2 y2 B x y = exp ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Solns_Q_1-8.pdf -- 147.7 Кб -- 18.03.2015
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    5. http://www.mso.anu.edu.au/~charley/papers/DaviesDavisLineweaver.pdf
    ... Total transportation distances ranged from 34 to 55 m (44.4 8.7 m; n 5). ... glide, the snake took off with a maximum upward acceleration of 14.4 0.8 m s 2 (mean s.e.m.) and horizontal velocity of 1.7 0.1 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/DaviesDavisLineweaver.pdf -- 115.1 Кб -- 11.12.2004
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    6. Siding Spring Survey Follow-up Obs
    ... Follow-up astrometry and recoveries are made with the ANU 40 inch (1.0-m) f/8 reflector at Siding Spring Observatory (IAU code 413). ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~rmn/follow-u.htm -- 13.0 Кб -- 16.02.2005
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    7. http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L08/Lecture08.pdf
    ... t = 0+0в0.1 = 0 ­ New value of v is k 5 v + g - x t = 0 + 9.8 - 0 в 0.1 = 0.98 m 0.1 Tuesday, 8 March 2011 So after 0.1 seconds ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L08/Lecture08.pdf -- 1087.3 Кб -- 08.03.2011
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    8. GSAOI Magellanic Cloud Planetary Nebulae Science Page
    ... Theoretical evolutionary tracks predict that all stars with masses in the range 1.4-8 M Sun should become PNe. ... to 0.6 M Sun , except for a few Peimbert Type I nebulae (e.g., NGC 6302 with 0.8 M Sun , or a handful of objects in the LMC ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gsaoi/science/pne.shtml -- 8.4 Кб -- 01.10.2012
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    9. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Battaglia06
    ... Bosma (1978) found a total H I mass of 2.8 в107 M (with a distance of 7.2 Mpc ... pc-3 , rc = 8.4 ± 1.4 kpc, and M/L = 3.8 ± 0.1 in F band, corresponding to a M/L in ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Battaglia06 -- 762.9 Кб -- 22.03.2007
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    10. http://www.mso.anu.edu.au/~kcf/pubs_top20/27.pdf
    ... 0.27 Jy at 3.6 m, 0.4 Jy at 4.5 m, 2.7 Jy at 5.8 m, and 2.5 Jy at 8.0 m. From the observed afterglow spectral index, ј ю1:25 (F ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/27.pdf -- 711.2 Кб -- 16.10.2011
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