http://arxiv.org/abs/2211.12297
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.
B. Poggianti and G. team
Wed, 23 Nov 22
54/71
Comments: 10 pages, 8 figures, proceedings of IAUS373: Resolving the rise and fall of star formation in galaxies, eds. W.-T. Kim & T. Wong – invited talk – after reviewer revisions
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