Abstract
For the first time in any ram pressure stripped galaxy, we detect large
amounts of cold molecular gas in the X-ray bright, and star forming tail
of ESO 137-001 in the Norma cluster. We find very low star formation
efficiency in the stripped gas, similar to values found in the outer
spiral disks where however molecular gas is mostly undetected. The
results were recently published in Jáchym et al. (2014).
Original language | English |
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Pages (from-to) | 227-229 |
Journal | Proceedings of the International Astronomical Union |
Volume | 309 |
DOIs | |
Publication status | Published - 1 Feb 2015 |
Externally published | Yes |