Table 1: SFRs (Cols. 2 and 3) and SFR densities (Cols. 4 and 5) of the discovered UCNR, as determined from the H$\alpha $ and UV images. Foreground dust extinction of $A_{{\rm H}\alpha }=A_{\rm UV}=2$ mag was assumed in all cases.
Galaxy $\rm {H}\alpha$ $(M_{\odot}~\rm {yr}^{-1})$ UV $(M_{\odot}~\rm {yr}^{-1})$ $\rm {H}\alpha$ $(M_{\odot}~\rm {yr}^{-1} \rm {pc}^{-2})$ UV $(M_{\odot}~\rm {yr}^{-1}~\rm {pc}^{-2})$
NGC 2985 0.026 0.050 $1.8 \times 10^{-6}$ $3.4 \times 10^{-6}$
NGC 4579 0.042 0.064 $1.5 \times 10^{-6}$ $2.3 \times 10^{-6}$
NGC 4800 (inner UCNR) 0.00063 - $2.7 \times 10^{-7}$ -
NGC 4800 (outer UCNR) 0.030 - $6.0 \times 10^{-7}$ -


Source LaTeX | All tables | In the text