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Home All issues Volume 500 / No 3 (June IV 2009) A&A, 500 3 (2009) 1287-1325 Full HTML
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Table 4:

Weights of stellar populations obtained by modelling of OASIS data, and compared to Cid Fernandes et al. (2004), on aperture ${\sim }1\hbox {$^{\prime \prime }$ }$. The symbols  $\mu _{\rm Y},\mu _{\rm I},\mu _{\rm O}$ denote mass fractions of young, intermediate and old populations, respectively. Analogously for $\mu _{\rm young}$, $\mu _{\rm old}$ in our OASIS data.
Galaxy OASIS data Cid Fernandes et al. (2004)
  $\mu _{\rm young}$ $\mu _{\rm old}$ $\mu_{\rm Y}$ $\mu_{\rm I}$ $\mu_{\rm O}$
NGC 2992 0.09 0.91 0.0000 0.0260 0.9740
NGC 3081 0.008 0.992 0.0000 0.0000 1.0
NGC 4388 0.02 0.98 0.0002 0.0000 0.9998
NGC 5728 0.06 0.94 0.0002 0.0699 0.9299

Source LaTeX | All tables | In the text

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