Sample
The MAUVE sample consists of 40 late-type galaxies in the Virgo Cluster targeted with the MUSE instrument on the ESO VLT, for which ALMA observations of the molecular gas content are already available from the VERTICO survey. We show below the 37 galaxies targeted by this program (3 already have MUSE archival data), with MUSE pointings in cyan (or orange, if from archival data) overlaid on optical images from the Sloan Digital Sky Survey, and contours of CO(2-1) emission tracing molecular gas from VERTICO.IC3392 |
NGC4064 |
NGC4189 |
NGC4192 |
NGC4216 |
NGC4222 |
NGC4293 |
NGC4294 |
NGC4298 |
NGC4302 |
NGC4330 |
NGC4351 |
NGC4380 |
NGC4383 |
NGC4388 |
NGC4394 |
NGC4396 |
NGC4402 |
NGC4405 |
NGC4419 |
NGC4424 |
NGC4450 |
NGC4457 |
NGC4501 |
NGC4522 |
NGC4548 |
NGC4567, NGC4568 |
NGC4569 |
NGC4579 |
NGC4580 |
NGC4606 |
NGC4607 |
NGC4654 |
NGC4689 |
NGC4694 |
NGC4698 |