... Narrow-band photometry of the Orion Sword" M.S.S.S.O.Preprint, Oct 17, 1-20, 1972 ... and autoguiding camera for the ANU 2.3 m Telescope", PASA, 17, 102, 2000 162 ... Bessell, M.S. "Beauty and Astrophysics", PASP, 17, 179, 2000 168. ...
... 12) High Energy Astrophysics: Accretion Disks II 17/59 ~ M a rv ( r ) r 0 r As we ... 2 G r ( r ) 2 ~ = M a r 0 v ( r 0 ) + 2 r 0 Gr ( r 0 ) (1.5-17) tells us that Flux ...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/11_Accretion_Disks_II.pdf -- 813.5 Кб -- 12.06.2003 Похожие документы
... of the sky: (means that sky noise will be the dominant noise source). object < sky 4.9 в 10 6 < 1.1 2.5112 mm > 17 Therefore sky limited in B band for m>17th magnitude Counts=number of counts, t=exposure time 4.9 в106 Counts= (object+ sky) в t = 2.5112m ...
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Ссылки http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/74_inch_Telescope_Efficiency_Response.pdf -- 53.4 Кб -- 28.07.2010 Похожие документы
... pc = 3.09 10 m v = 1 000 km s н 1 = 10 6 m s н 1 Units 1 solar mass = 2 10 30 16 15 (16) kg 7 1 pc = 3.09 10 m (17) 1 year = 3.16 10 seconds The density of the wind at 0.1 pc from the star is: = 5.2 10 Fundamental equations н 22 kg m н 3 (18) 10/78 This ...
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Ссылки http://www.mso.anu.edu.au/~geoff/AGD/Fundamental_Equations.pdf -- 1260.0 Кб -- 19.02.2016 Похожие документы
... have: dQ 4 = TEarth = Io (1 - AEarth ) (16) dt = 342 (0.7) Wm-2 = 238 W m-2 , where AEarth 0.3 is the albedo of the Earth, and the StefanBoltzmann constant is = 5.67 в 10 Thus the flux of free energy through unit area (Eq. (14)) is -8 m-2 (17) Wm -2 K -4 ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/LineweaverEgan2008v2.pdf -- 826.4 Кб -- 18.03.2009 Похожие документы