The detection of [Ne v] emission in five blue compact dwarf galaxies
  We report the discovery of the high-ionisation [Ne v] 3426A emission line in
the spectra of five blue compact dwarf (BCD) galaxies. Adding the three
previously known BCDs with [Ne v] emission, the entire sample of such galaxies
now contains eight objects. The detection of this line implies the presence of
intense hard ionising radiation. Such radiation cannot be reproduced by models
of high-mass X-ray binaries or massive stellar populations. Other mechanisms,
such as AGN and/or fast radiative shocks, are needed. We consider that fast
radiative shocks is the most likely mechanism. The observed [Ne v] 3426/He ii
4686 flux ratios in all eight galaxies can be reproduced by radiative shock
models with shock velocities in the ~300-500 km/s range, and with the shock
ionising contribution being ~10% of the stellar ionising contribution. However,
we cannot rule out that this 10% part is produced by an AGN rather than by
radiative shocks.
