... McClure-Griffiths, N.M., Gaensler, B.M., Green, A.J., Haynes, R.F., & Wieringa, M.H. 2000, in Radio Polarization: A New Probe of the Galaxy, ed. T.L. Landecker, p. 43. ...
... Dupuis, J., Vennes, S., Chayer, P., Hurwitz, M., and Bowyer, S., 1998, "Properties of the Hot DA White Dwarf HZ 43 Based on Far-Ultraviolet ORFEUS-SPAS II Observation", The Astrophysical Journal Letters, 500, 45-49. ...
... If M(B AB ) is related to L(H alpha) at z = 1 as it is at z < 0.3, then L * H alpha = 10 42.73 erg s -1 at z = 1. ... The median L(H alpha) at 0.75 < z < 1.9 is 10 42.43 erg s -1 from slitless grism spectroscopy with NICMOS. ...
... Gi ve n t h at t h e gove r n m e nt h a s s p e nt AUS$43.5 million on the ERA, and universities themselves have outlaid substantial sums to undertake the ERA evaluations since 2008, one might question the value of this exercise that awards so little ...
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Ссылки http://www.mso.anu.edu.au/~brian/IMAGES/Nature-july2014.pdf -- 349.6 Кб -- 24.07.2014 Похожие документы
... 1-2) 3 where the electron radius, 15 e2 r 0 = ------------------------- = 2.818 в10 m 4 0 m e c 2 (3.1-3) High Energy Astrophysics: Accretion Disks II 43/59 Calculation of momentum flux density The momentum flux density per unit frequency is given by: 1 ...
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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
... Q ЁP 4I № є HE YХ U» GF ¦E РФ DC а ю w zm ¤ fm Bс w u ¦~ w Uф #ж u ¦ю ¦w 5 #~ ¤y ¤m Ї} $~ 'u '~ { Ёj u ¤m ¤} Fm г $m $ I ю а с Ё} vu ¤j Fm ¦е К ¤{ 2m ~ u 'ю 43 ¤} zm q { $д vw г 5y dю е W 5 y 5y ¤j Ёm u 5n б~ d~ бе @y } $r w ¤y р $y '~ n ¤y $m iw хj Ёj Wu ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/SchwartzmanLineweaverHamilton.pdf -- 288.7 Кб -- 09.04.2003 Похожие документы