  We present an analysis of the kinematics and ionization conditions in a
sample composed of seven star-forming galaxies undergoing ram-pressure
stripping in the A1367 cluster, and the galaxy ESO137-001 in the Norma cluster.
MUSE observations of two new galaxies in this sample, CGCG097-073 and
CGCG097-079, are also presented. This sample is characterized by homogeneous
integral field spectroscopy with MUSE and by a consistent selection based on
the presence of ionised gas tails. The ratio [OI]/H${\alpha}$ is consistently
elevated in the tails of these objects compared to what observed in unperturbed
galaxy disks, an ubiquitous feature which we attribute to shocks or turbulent
phenomena in the stripped gas. Compact star-forming regions are observed in
only $\approx$ 50% of the tails, implying that specific (currently unknown)
conditions are needed to trigger star formation inside the stripped gas.
Focusing on the interface regions between the interstellar and intracluster
medium, we observe different line ratios that we associate to different stages
of the stripping process, with galaxies at an early stage of perturbation
showing more prominent signatures of elevated star formation. Our analysis thus
demonstrates the power of a well selected and homogeneous sample to infer
general properties arising from ram-pressure stripping inside local clusters.
