The high molecular gas content, and the efficient conversion of neutral into molecular gas, in jellyfish galaxies
A. Moretti, R. Paladino, B. M. Poggianti, P. Serra, M. Ramatsoku, A., Franchetto, T. Deb, M. Gullieuszik, N. Tomicic, M. Mingozzi, B. Vulcani, M., Radovich, D. Bettoni, J. Fritz

TL;DR
This study reveals that jellyfish galaxies at low redshift have significantly higher molecular gas content and lower star formation efficiency due to ram pressure stripping, which efficiently converts neutral hydrogen into molecular gas.
Contribution
It provides the first detailed analysis showing that ram pressure stripping in jellyfish galaxies enhances molecular gas content by converting neutral hydrogen, with implications for galaxy evolution.
Findings
Molecular gas masses are 4-5 times higher than in similar non-stripped galaxies.
Molecular gas depletion times range from 1 to 9 Gyr, indicating low star formation efficiency.
Total gas content is similar to normal spirals, but with a higher molecular to neutral gas ratio.
Abstract
In the disks of four jellyfish galaxies from the GASP sample at redshift we detect molecular gas masses systematically higher than in field galaxies. These galaxies are being stripped of their gas by ram pressure from the intra cluster medium and are, in general, forming stars at high rate with respect to non-stripped galaxies of similar stellar masses. We find that, unless giant molecular clouds in the disk are unbound by ram pressure leading to exceptionally high CO--to-- conversion factors, these galaxies have a molecular gas content 4-5 times higher than normal galaxies of similar masses, and molecular gas depletion times ranging from 1 to 9 Gyr, corresponding to generally very low star formation efficiencies. The molecular gas mass within the disk is a factor between 4 and 100 times higher than the neutral gas mass, as opposed to the disks of normal…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
