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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 3:

Comparison of our emission fluxes with those of Falcke et al. (1998). OASIS values correspond to fluxes corrected for absorption using a combination of SSPs as described in Sect. 3.1. Units are $10^{-19}~{\rm W~m}^{-2}$.
Galaxy Aperture OASIS data Falcke et al. (1998)
  radius [O III] H$\alpha$ + [N II] [O III] H$\alpha$ + [N II]
Mrk 34 2 $^{\prime\prime}$ 4800 3400 6100 3600
  0.5 $^{\prime\prime}$ 500 300 1300 700
Mrk 348 1.5 $^{\prime\prime}$ 3000 2500 4100 2000
  0.4 $^{\prime\prime}$ 1500 1000 3200 1500
NGC 4388 6 $^{\prime\prime}$ 9800 -- 11 700 --
  1 $^{\prime\prime}$ 3200 -- 3900 --

Source LaTeX | All tables | In the text

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