
science & techESA/Hubble
A galaxy trailing star-forming tendrils shows how a cluster's hot gas can strip a galaxy
The jellyfish galaxy JW39 lies about 900 million light-years away in Coma Berenices and is moving through a galaxy cluster. Clusters are full of a very hot, thin plasma called the intracluster medium. As a galaxy moves through it, the gas acts like a headwind, pushing gas and dust out of the galaxy's disc. This process is called ram-pressure stripping, and it leaves long trailing ribbons that resemble jellyfish tentacles. Hubble's Wide Field Camera 3 studied these tails and found that star formation in the tentacles is not noticeably different from star formation in the galaxy's disc. Stripping leaves a galaxy with less gas to make new stars, so its star formation eventually slows.
A galaxy moving through the intracluster plasma feels a pressure that pushes against its gas. Where that pressure exceeds the gravity holding the gas in place, the gas is stripped away and streams behind the galaxy.
The study shows that star formation can continue in the extreme conditions of stripped gas, which challenges assumptions about where stars can form. Jellyfish galaxies also provide a natural laboratory for how galaxies die out in dense clusters.
Galaxies in clusters are shaped by their environment, including gravitational tugs and gas stripping. Studies of interacting and stripped galaxies have been a major theme in extragalactic astronomy for decades.
ESA/Hubble · CC BY 4.0
Image: ESA/Hubble & NASA, M. Gullieuszik and the GASP team
