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    61. Proposed Facility
    ... What is needed, therefore, is an infra-red multi-object spectrograph on an 8-m class telescope (or preferably several of them). ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node7.html -- 3.6 Кб -- 02.10.2012
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    62. http://www.mso.anu.edu.au/~brian/A3002/lect15.pdf
    ... s a r e d e r i m a s k in g b r ig h t s o u r c e s a n d s u b tr s p e c tr a l te m p la te s fo r th e v a r io u s 4 0 8 M H z s y n c h r o tr o n r a d ia tio n , v e d fro m a m a p b a s e d o n a c tin g fo r e g r o u n d s b a s e d o n c o ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~brian/A3002/lect15.pdf -- 2186.3 Кб -- 28.08.2007
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    63. http://www.mso.anu.edu.au/pfrancis/roleplay/MysteryPlanet/answer23.pdf
    ... From these masses and radii we can work out the surface gravity g, using the equation GM g= 2 r 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. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/MysteryPlanet/answer23.pdf -- 106.0 Кб -- 17.03.2004
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    64. http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/SKA_Forum_2010.pdf
    ... Blue Galaxies Outside X-ray Gas HI 21cm emission at z > 0.1 Telescope WSRT VLA Redshift z = 0.18 Abell 2218 z = 0.19 Abell 2192 Obs Time 200 hours ~80 hours Number and HI Mass of galaxies 1 galaxy 4.8 109 M 1 galaxy 7.0 109 M Who and When Zwaan et al ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/SKA_Forum_2010.pdf -- 2113.2 Кб -- 28.07.2010
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    65. http://www.mso.anu.edu.au/~kcf/pubs_top20/34.pdf
    ... High signal-to-noise 8-m spectra will be required on the distilled sample of extremely metal-poor stars for detailed elemental abundance studies. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/34.pdf -- 664.4 Кб -- 15.10.2011
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    66. http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L08/iteration_spring.py
    ... Delta_t = 0.1 g = 9.8 k = 10.0 m = 1.0 t = 0 v = 0 x = 0 while t < 10.0: t = t + Delta_t x = x + v*Delta_t v = v + (g-k*x/m)*Delta_t print t, x. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L08/iteration_spring.py -- 1.2 Кб -- 08.03.2011
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    67. http://www.mso.anu.edu.au/pfrancis/roleplay/MysteryPlanet/Answers_23.doc
    ... From these masses and radii we can work out the surface gravity g, using the equation [pic] 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. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/MysteryPlanet/Answers_23.doc -- 51.5 Кб -- 17.03.2004
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    68. http://www.mso.anu.edu.au/~charley/papers/LineweaverEgan2008v2.pdf
    ... 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 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/LineweaverEgan2008v2.pdf -- 826.4 Кб -- 18.03.2009
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    69. http://www.mso.anu.edu.au/~kcf/surya/Sellwood.Deb06.pdf
    ... The solid lines are from our runs F & S, reproduced from Fig. 1, in which sectoral harmonics 0 m 8 contributed to the forces computed from the disk particles. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/Sellwood.Deb06.pdf -- 432.4 Кб -- 31.07.2007
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    70. Mass Feeding and Feedback in Young Stellar Objects
    ... Peter McGregor has built the NIFS adaptive-optics-corrected integral-field spectrograph on the 8-m diameter Gemini North telescope. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~raquel/TTauri.html -- 4.7 Кб -- 01.10.2012
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