Unveiling the Interplay between the GASP Jellyfish Galaxy JO194 and Its Environment with Chandra

X-ray studies of jellyfish galaxies opened a window in the physics interplay between intracluster medium (ICM) and interstellar (ISM). In this paper, we present study an archival \textit{Chandra} observation GASP galaxy JO194. We observe emission extending from stellar disk to unwinding spiral arms with average temperature $kT=0.79\pm0.03$ keV. To investigate origin emission, compare observed luminosities those expected star formation rates (SFR) obtained H$\alpha$ emission. estimate luminosity excess factor $\sim2-4$ respect SF, therefore conclude that SF is not main responsible for extended The metallicity ($Z=0.24^{+0.19}_{-0.12} Z_{\odot}$) consistent ICM around JO194 ($Z=0.35\pm0.07$), thus suggest radiative cooling dominates arms. speculate plasma results ISM-ICM interplay, although nature still mostly unknown. Finally, properties are two other different mass, phase-space conditions their hosting clusters, local conditions. required induce established at beginning stripping, they can persist on long time scales so clusters evolutionary stages similar