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    1. Siding Spring Survey Follow-up Obs
    ... c) ANU/RSAA 2003 . Discovery of 2003 XB22 on 2003 Dec 15 with the 1.0-m at SSO . ... c) ANU/RSAA 2003 . 2004 CB on 2004 Mar 30, imaged with the 1.0-m at SSO . ... made with the ANU 40 inch (1.0-m) f/8 reflector at Siding Spring Observatory (IAU ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~rmn/follow-u.htm -- 13.0 Кб -- 16.02.2005
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    2. http://www.mso.anu.edu.au/~geoff/HEA/Q1-4.pdf
    ... 2.41 10 ------ Hz ­ 34 eV eV h 6.62 10 hc hc ­6 = ----- = ----- = 1.24 10 ------ eV ­1 4 m = 1.24 10 ------ eV ­1 ­ 19 ­ 34 8 ­1 eV Angstroms Hence the following table (the primary quantity is given in bold): Photon Typical microwave Typical far infrared ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Q1-4.pdf -- 117.5 Кб -- 04.08.2009
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    3. http://www.mso.anu.edu.au/~brian/A3002/probset1.pdf
    ... Cosmological constant, no photons, and nothing else of interest, the k=-1 solution of the Friedman equations is given by: a M = (cosh 1) a0 2(1 M) 1 M t= (sinh ) 3/ 2 H 0 2(1 M) Problem 3: (3pts) Assuming a matter-dominated Universe (as above) and a value ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~brian/A3002/probset1.pdf -- 262.1 Кб -- 02.09.2009
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    4. http://www.mso.anu.edu.au/~brian/A3002/lect4.pdf
    ... Out the Equation of State w" p #c 2 "!V #i a 3wi + 3 = constant 3w + 3 $ # '$ a ' & )& ) % # 0 (% a0 ( =1 &M $ & ) # $M ... dt y ln( y ) = H 0 t y=e H0t 2 2 2 ) rad a = = (1 + z ) )M a0 )" ( a =& ) M & a0 ' % # = (1 + z ) # $ !3 !3 · · · N o te th a t ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~brian/A3002/lect4.pdf -- 525.5 Кб -- 03.10.2006
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    5. http://www.mso.anu.edu.au/pfrancis/ObsTech/MagPrac.pdf
    ... What is its flux at this wavelength: · In f · In f (answers: 4.48в10 -2 0 W m-2 nm-1, 1.16в10 -3 1 W m-2 Hz-1). ... f) flux in V? and in I? What is the ratio between the two? (answers: 1.45в10 -1 9 W m-2 nm-1, 5.91в10 -2 0 W m-2 nm-1, 2.45 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/ObsTech/MagPrac.pdf -- 60.0 Кб -- 13.04.2007
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    6. Siding Spring Survey 2004 CB
    ... P/2004 CB (LINEAR) . 2004 CB on 2004 Mar 30, imaged with the 1.0-m at SSO . ... During routine astrometry with the 1.0-m to improve the orbit of the Apollo asteroid ... Discoveries . Follow-up Astrometry with the 1.0-m at SSO . Previous News Items . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~rmn/2004cb.htm -- 5.6 Кб -- 16.02.2005
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    7. http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/questacon_2011.pdf
    ... for my research Atmospheric Transmission optical gamma rays, X-rays & ultravio let infrared radio Atmospheric Opacity 100 % 50 % 0% 1 nm 1 m 1 mm 1m 1 km Wavelength Frequency Hydrogen Gas in the Universe Hydrogen Gas in the Universe Hydrogen 76% by mass ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/questacon_2011.pdf -- 2383.4 Кб -- 19.05.2011
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    8. GSAOI Magellanic Cloud Planetary Nebulae Science Page
    ... tracks predict that all stars with masses in the range 1.4-8 M Sun should become PNe ... of the PN is typically of order 0.1 M Sun , and the derived mass is found to depend ...
    [ 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/~geoff/HEA/Q10-13.pdf
    ... 2 2 mJy arcsec mJy arcsec ­2 W m 1 -------- ----------- 180 3600 I used the plotted ... 12 N m ­ 2 10 7 10 ­1 ­1 m ­3 p tot,min T ­3 = 7.2 10 ... this energy is given by E where we take 0.1 Thus, M acc,min min = M acc,min c 2 5 10 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Q10-13.pdf -- 137.0 Кб -- 22.09.2009
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    10. http://www.mso.anu.edu.au/~geoff/HEA/Questions%201-8.pdf
    ... is hc 6.62 10 3.0 10 = ----- = ---------------------------------------------------- = 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 = -- = ------------------------- 34 h 6.62 10 hc ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Questions%201-8.pdf -- 138.6 Кб -- 09.09.2011
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