Original title: Určování rozložení hmoty v jádře Galaxie z pohybů hvězd
Translated title: Determination of the mass distribution in the Galactic centre from the stellar motions
Authors: Schovancová, Jaroslava ; Šubr, Ladislav (advisor) ; Mayer, Pavel (referee)
Document type: Master’s theses
Year: 2007
Language: cze
Abstract: We present an implementation of the statistical approach to the stars-gas mass exchange cycle into an N-body code. First, we summarize available data on stellar mass-loss and derive the time-dependency of the mass-loss rate of a single stellar population. Since the adopted probabilistic scheme that served as a basis for our implementation was limited to the linear star formation law while observations seem to suggest a non-linearity, we derive the non-linear star formation scheme. Both sides of the mass exchange cycle are then implemented into the code with stellar and gaseous particles and compared with an analytic recipe to test their reliability. In the next step, the comparison of such an extended statistical approach with deterministic scheme is performed for a fully dynamical model. The aim of the comparison is to explore divergence between both models of different natures. As an illustration of the code application and sensitivity of the resulting galaxy disk dynamics, several comparisons with varying the key parameters are performed.

Institution: Charles University Faculties (theses) (web)
Document availability information: Available in the Charles University Digital Repository.
Original record: http://hdl.handle.net/20.500.11956/12623

Permalink: http://www.nusl.cz/ntk/nusl-288440


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Universities and colleges > Public universities > Charles University > Charles University Faculties (theses)
Academic theses (ETDs) > Master’s theses
 Record created 2017-04-25, last modified 2022-03-04


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