Non-star-forming molecular gas in the Abell 1367 intra-cluster multiphase orphan cloud

We report the detection of CO emission in recently discovered multiphase isolated gas cloud nearby galaxy cluster Abell 1367. The is located about 800 kpc projection from center and at a projected distance > 80 any galaxy. It first only known intra-cluster detected X-ray, H$\alpha$, emission. found total $2.2\times 10^8 M_\odot$ H$_2$ with IRAM 30-m telescope two regions, one associated peak H$\alpha$ another X-ray surrounded by weak filaments. velocity molecular offset underlying 100 km s$^{-1}$ region where peaks. may account for 10% cloud's mass, which dominated hot component. previously measured upper limit on star formation rate indicates that component non-star-forming state, possibly due to combination low density observed level dispersion. presence three phases suggests phase mixing surrounding medium taking place. possible origin orphan late evolutionary stage ram pressure stripping event. In contrast, stripped 2MASX J11443212+2006238 an early we $2.4\times 10^9 its main body.