A massive outflow from NGC 4383
The first paper from the MAUVE survey! We charactersied the kinematic and chemical properties of a massive ionised gas outflow from NGC 4383.
The gas reservoirs of galaxies participate in a complex cycle of consumption to form new stars, replenishment from pristine gas inflows, and heavy element-enriched feedback from dying stars. However, galaxies are rarely able to recover a reservoir of star-forming gas once it it is gone.
Understanding how, and why, galaxies lose their star-forming gas is essential to understanding galaxy evolution.
I am currently working on several research projects, including:
The first paper from the MAUVE survey! We charactersied the kinematic and chemical properties of a massive ionised gas outflow from NGC 4383.
Using sub-kpc observations, we show that the atomic and molecular gas within the truncation raidus of ram pressure stripped galaxies also systematiclly suppr...
A journey through asymmetry in neutral atomic hydrogen from deep HI data, numerical simulations, and combination with IFS data from the SAMI survey.