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Ссылки http://www.atnf.csiro.au/research/Astro2010/talks/mverdon.pdf -- 553.5 Кб -- 16.06.2010 Похожие документы
... Series Vol. 106, ed. Evan Skillman, p. 238).. ... Recent measurements with the ATCA 375-m array revealed an HI bridge between the two ... These data have been obtained with the 375-m array of the ATCA (12 h). ...
... Writing the integral in (3) in the form L ne B cos and expressing L in parsecs, ne per cubic centimetre and B in gauss, (3) becomes RM = 0 · 8 в 106 L ne B cos rad m-2 . ...
... sin sin i, (2) 2 f x dx 0 (x ) 2 B , (1) (x ) where 0 is the initial Lorentz factor, c = h/m Ї e c is the Compton wavelength, = 1 · 686 в 10-4 (T/106 K) is the effective temperature (in me c2 ), R0 is the star's radius, T is the Thomson cross section, f 1 ...
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Ссылки http://www.atnf.csiro.au/whats_on/workshops/synthesis2003/talks/galaxies.pdf -- 1410.4 Кб -- 22.05.2003 Похожие документы
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