... Thus, the expected BHmass in NGC 4041 would be 1:2 # 10 7 M # , in agreement with ... et al. 2002) or M BH ј 1:4 # 10 8 П# # =200 km s #1 ч 4:8 (Merritt & Ferrarese 2001a ...
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Ссылки http://www.stsci.edu/~marel/abstracts/psdir/2003ApJ...586..868M.ps -- 2672.7 Кб -- 30.03.2003 Похожие документы
... distribution of formal uncertainties (oe п(ff) ; oe п(ffi) ; oe ‹ ) as a function of ... п Y (T \Gamma T 0 ) + F Y ‹ (4) where (X, Y) are the observations, (X 0 ; Y 0 ) the ...
... NGC 5194 are bracketed by models of stellar populations in the age range 2 300 Myr, with dust extinction AV P 2:8 mag, for our adopted dust model. variation driven by the aging of a dust-free stellar population, the conversion formula would be logЅLk ...
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Ссылки http://www.stsci.edu/~mutchler/documents/ApJ_2005_SINGS_M51a.pdf -- 1188.7 Кб -- 07.11.2005 Похожие документы
... NGC 4676 NGC 4676 is a low-redshift pair of merging spiral galaxies and was observed ... 0:25re ю 0:013: П 3ч ј zBPZ Ч 0:045 ; (1 ю 0:045) П 1ч is plotted against zspec in ...