The role of dry mergers in shaping the scaling relations of galaxies
Mauro D'Onofrio, Cesare Chiosi, Francesco Brevi

TL;DR
This paper develops a simple dry merger theory based on the scalar Virial Theorem to explain galaxy scaling relations, successfully matching observational data and detailed simulations across cosmic time.
Contribution
It introduces a novel, rapid theoretical model of dry mergers that accurately reproduces galaxy scaling relations and their evolution, complementing complex numerical simulations.
Findings
Dry mergers explain observed galaxy scaling relation characteristics.
The model matches data across different cosmic epochs.
It offers a fast alternative to detailed simulations.
Abstract
In the context of the hierarchical formation of galaxies, we investigated the role played by mergers in shaping the scaling relations of galaxies, that is the projections of their Fundamental Plane onto the Ie-Re, Ie-Sigma, Ms-Re and L-Sigma planes. To this aim, based on the scalar Virial Theorem, we developed a simple theory of multiple dry mergers to read both the large scale simulations and the companion scaling relations. The aim was to compare the results of this approach with the observational data and with two of the most recent and detailed numerical cosmo-hydro-dynamical simulations, that is Illustris-TNG and EAGLE (Evolution and Assembly of GaLaxies and their Environments). We derived the above scaling relations for the galaxies of the MaNGA (Mapping Nearby Galaxies at APO) and WINGS (Wide-field Imaging of Nearby Galaxy-Clusters Survey) databases and compared them with the…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stochastic processes and financial applications · Modeling, Simulation, and Optimization
