The spatially resolved view of star formation in galaxy clusters by Bianca M. Poggianti et al. on Thursday 24 November

Integral field spectroscopic studies of galaxies in dense environments, such

as clusters and groups of galaxies, have provided new insights for

understanding how star formation proceeds, and quenches. I present the

spatially resolved view of the star formation activity and its link with the

multiphase gas in cluster galaxies based on MUSE and multi-wavelength data of

the GASP survey. I discuss the link among the different scales (i.e. the link

between the spatially resolved and the global star formation rate-stellar mass

relation), the spatially resolved signatures and the quenching histories of

jellyfish (progenitors) and post-starburst (descendants) galaxies in clusters.

Finally, I discuss the multi-wavelength view of star-forming clumps both in

galaxy disks and in the tails of stripped gas.

arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.12297v1