Structure and Evolution of Regular Galaxies
Jaan Einasto

TL;DR
This paper synthesizes data on galaxy structure, kinematics, and evolution to develop models of the Milky Way and Andromeda, revealing limitations in reproducing observed galaxy rotation curves with known stellar populations.
Contribution
It introduces new methods for modeling galaxy structures and their evolution, integrating observational data with physical models, and provides detailed galaxy models and evolutionary theories.
Findings
Developed spatial and hydrodynamical models of the Galaxy and M31.
Reconstructed the Galaxy's dynamical evolution using stellar kinematics.
Concluded that known stellar populations cannot fully explain observed galaxy rotation curves.
Abstract
The Thesis is an attempt to combine data from three previously independent areas - the structure and kinematics of stellar populations of the Galaxy, photometric and dynamical models of galaxies, and models of the dynamical and physical evolution of galaxies. This synthesis was made with the goal to understand better the vast topic of the structure and evolution of galaxies. The main results of the study can be divided into methodical and astronomical. The methodical results are 1) extrapolation of the mass distribution function beyond the Sun distance, and the determination of the circular velocity at the Sun distance from the Galactic centre; 2) conditions of physical correctness of models are developed, and the generalised exponential model is suggested; 3) a method has been developed to construct spatial and hydrodynamical models of stellar systems, using a combination of…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
