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    61. http://www.mso.anu.edu.au/~micheleb/images/TNO2010_abstract_MTB.pdf
    ... ecliptic that have more than thirty nights of observation over five years, with an approximate limiting flux of m(clear ) 19.5 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~micheleb/images/TNO2010_abstract_MTB.pdf -- 30.5 Кб -- 02.12.2010
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    62. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Rautiainen04
    ... 200 km s-1 150 100 50 0 0 20 r [arcsec] 40 60 15 10 M 5 0 0 20 r [arcsec] 40 60 H, dominating halo 250 km s-1 arcsec -1 H 15 10 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Rautiainen04 -- 1663.8 Кб -- 09.07.2007
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    63. http://www.mso.anu.edu.au/~gdc/prepr/GDaC_Dunk2001.pdf
    ... x z hЉ U‡ rµ U‡ Ё "} 9‡ јz м¬ CІ ~ y­ $z €І 0« g№ €z ёx 5« sѓ m„ r¦ № 0« мІ €І Ѓ '} 3­ и• Ѓ 5Ї Ѓ WЂ z 0« 'І z Ѓ ЌІ в№ и– ж© y ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~gdc/prepr/GDaC_Dunk2001.pdf -- 711.0 Кб -- 27.08.2002
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    64. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/kranz01.pdf
    ... NGC 4254 with a total exposure time of 20 minutes at the Calar Alto 3.5 m telescope ... All data were acquired at the Calar Alto observatoryоs 3.5 m telescope. ... with the Omega Prime camera at the 3.5 m telescopeоs prime focus (Bizenberger et al ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/kranz01.pdf -- 2023.5 Кб -- 09.07.2007
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    65. 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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    66. http://www.mso.anu.edu.au/~kcf/pubs_top20/34.pdf
    ... SkyMapper is a 1.3-m telescope featuring a 5.7-square-degree field-of-view Cassegrain imager commissioned for the Australian ... 2.2 Enclosure The SkyMapper enclosure is 6.5 m in diameter and 11 m high with three internal levels as shown in Figure 2. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/34.pdf -- 664.4 Кб -- 15.10.2011
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    67. http://www.mso.anu.edu.au/~kcf/surya/bars/Perez04
    ... We adopted a Salpeter IMF with a flatter slope for m< 0.5 M . ... kinematics obtained through long slit spectroscopy at the 1.5 m at La Silla Observatory show a very complicated rotation curve ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/bars/Perez04 -- 1671.5 Кб -- 13.12.2006
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    68. http://www.mso.anu.edu.au/~raquel/GRC_poster_5.pdf
    ... well mixed with the gas. (b) Conductivity regime (b1) R = 5 AU, 3 m grains Hall diffusion modifies the most unstable MRI modes ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~raquel/GRC_poster_5.pdf -- 1425.4 Кб -- 13.09.2007
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    69. http://www.mso.anu.edu.au/~geoff/AGD/Sedov.pdf
    ... by the supernova. r BW 5 E = 0 -----------t2 / 5 5 = 0 ­ 5 r BW t ­ 2 (67) Take ISM number density n 1 cm ­ 3 10 6 m ­ 3 5 E nm ­ 5 r BW t ­ 2 = 5.8 10 42 n -------- J 10 6 r BW 5 t ­2 ----------------------- pc 100 yrs (68) Astrophysical Gas Dynamics ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/AGD/Sedov.pdf -- 231.6 Кб -- 29.05.2012
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    70. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Conselice05
    ... stellar mass Tully-Fisher relation in nearby disks, M V 4.5 (Bell & de Jong 2001 ... Figure 5 shows the distribution of f = M /Mhalo for systems more massive than, and ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Conselice05 -- 240.6 Кб -- 19.12.2006
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