Galactic Scaling Rules in a Modified Dynamical Model
Hossein Shenavar

TL;DR
This paper investigates galactic scaling laws within a modified dynamical framework, deriving relations through theoretical analysis and validating them with observational data, revealing insights into galaxy evolution and the applicability of these laws.
Contribution
The work introduces a modified dynamical model to derive and validate galactic scaling relations, including the baryonic Tully-Fisher relation, using a combination of theoretical derivations and observational data analysis.
Findings
Scaling relations fit observational data well with proper equilibrium measures.
The baryonic Tully-Fisher and mass-size relations effectively describe galaxy characteristics.
Predicted evolution of galactic properties with redshift offers insights into cosmic evolution.
Abstract
Schulz (2017) galactic scaling rules, which include baryonic Tully-Fisher relation, have been surveyed in this work within the context of a modified dynamical model. These scaling relations are derived by employing the virial theorem and applying equilibrium and stability conditions. The scaling rules are also obtained by dimensional analysis of an integral relation between surface density and circular velocity of disk galaxies. To check the validity of the scaling relations based on observational data, we have defined, based on the properties of the model, the proper equilibrium size and equilibrium velocity of systems. By employing these measures of length and velocity, SPARC data ( Lelli et al. 2016a ) is used to analyze the results. The viability of the scaling relations is tested and it is shown that, compared to some other measures of length and velocity,…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Complex Systems and Time Series Analysis
