small to make statistically meaningful statements, we note that none of the galaxies of Hubble type later than Scd in this sample display a \[NeV\] line. ](f1.eps "fig:"){width="9cm"}]{}

[lclccccccc]{}\
\
& Distance & & T & M$_{B_T}^0$ & \[OIII\]/H$_{\beta}$ & \[OI\]/H$_\alpha$ & \[NII\]/H$_\alpha$ & \[SII\]/H$_\alpha$ & Optical\
& (Mpc) & & & & & & & & Class\
& (2) & & (4) & (5) & (6) & (7) & (8) & (9) & (10)\
\
\
NGC925 & 9.4 & SAB(s)d & 7 & -19.90 & 0.84 & 0.01 & 0.22 & 0.33 & H\
NGC1569 & 1.6 & IBm & 10 & -16.60 & 5.48 & 0.00 & 0.04 & 0.03 & H\
NGC2276 & 36.8 & SAB(rs)c & 5 & -21.08 & 0.15 & 0.01 & 0.35 & 0.18 & H\
NGC2903 & 6.3 & SAB(rs)bc & 4 & -19.89 & 0.10 & 0.01 & 0.34 & 0.19 & H\
NGC2976 & 2.1 & SAc pec & 5 & -16.31 & 1.42 & 0.01 & 0.31 & 0.18 & H\
NGC3034 & 5.2 & IAO spin & 90 & -19.72 & 0.36 & 0.01 & 0.56 & 0.18 & H\
NGC3077 & 2.1 & IAO pec & 