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Are dwarf galaxy properties a sequence of time or of environment?

Applicant Professorin Dr. Eva K. Grebel, since 1/2019
Subject Area Astrophysics and Astronomy
Term from 2018 to 2023
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 394551440
 
Final Report Year 2024

Final Report Abstract

We used survey data and cosmological simulations in order to systematically investigate what determines the properties of today's early-type dwarf galaxy population in groups and clusters. Early-type dwarf galaxies typically no longer form stars, are dominated by older stellar populations, are elliptical in appearance and do not show ordered rotation. They are usually found in regions of high galaxy density, suggesting that interactions might be responsible for their appearance. Were they transformed to their present state by their environment, and what were their characteristics in the past? Our observational studies of the Virgo, Fornax, and Hercules galaxy clusters conducted in this study all support environmental mechanisms such as ram pressure stripping or tidal stripping as the major agents of change. Some dwarf galaxies were identified as recent infallers into the cluster potential, and intriguingly they still show indications of disks and more recent star formation. The cosmological simulations analyzed in this project allow us to quantify the impact of environmental effects and to explore gas content, star formation, and quenching as a function of time as well as infall time, confirming the dominant effect of the environment on dwarf galaxy evolution and transformation. This project resulted in ten refereed publications, five of which were led by persons funded by the project.

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