Spatially-resolved stellar population properties of galaxies in voids with the CAVITY project
Galaxies in voids have been found to be of a later type, bluer, less massive, and to have a slower evolution than galaxies in denser environments (filaments and walls). However, the effect of the void environment on their stellar population properties is still unclear. We aim to address this question using 118 optical integral field unit datacubes
Conrado, A. et al.
Advertised on:
5
2025