MUSE sneaks a peek at extreme ram-pressure stripping events – V. Towards a complete view of the galaxy cluster A1367

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