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The spatially resolved view of star formation in galaxy clusters

Published online by Cambridge University Press:  09 June 2023

Bianca M. Poggianti Open the ORCID record for Bianca M. Poggianti [Opens in a new window]  and
the GASP team
Bianca M. Poggianti
Affiliation:
INAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, Italy email: bianca.poggianti@inaf.it
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Abstract

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.

Keywords

Galaxy evolutionstar formationbaryonic cyclegalaxy clusters
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 17 , Symposium S373: Resolving the Rise and Fall of Star Formation in Galaxies , August 2021 , pp. 163 - 172
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Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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