092065

X-ray tails of late-type cluster galaxies are rare. Detailed studies of thesesystems allow better understanding for ram-pressure stripping galaxy evolutionin clusters mixing of the stripped cold ISM with the hot ICM r^antmicro-physics and intracluster SF. Recently we discovered likely the longestX-ray tail ever known in the Virgo cluster. Our new Ha data also show thediffuse Ha emission in the same region spectroscopically confirmed to beassociated with the parent galaxy. We propose a new XMM observation to confirmthe X-ray tail and further explore the X-ray-Ha correlation in poor environmentto compare with that in rich cluster tails. Joint time with VLT/MUSE is alsorequested to study the kinematics and gas ionization conditions of the warm gas in the tail. [truncated! Please see actual data for full text]