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Table 7:

Derived properties of the observed knots using the extinction-corrected H$\alpha $ fluxes measured in the images from Gil de Paz et al. (2003).
ID $R_{\rm eq}$ I(H$\alpha $) L(H$\alpha $) Q(H$^{\circ}$) $M_{\rm ion}$ M(HII) SFR
  (arcsec) (10-14 erg s-1 cm-2) (1038 erg s-1) (1051 s-1) (105 $M_\odot$) (104 $M_\odot$) $M_\odot$/yr
A 1.64 1.25 4.91 3.59 7.16 3.64 0.004
B 2.94 4.83 19.0 13.9 27.6 14.1 0.015
C 2.65 3.96 15.6 11.4 22.7 11.5 0.012
D 1.43 1.10 4.33 3.16 6.31 3.21 0.003

Source LaTeX | All tables | In the text

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