We present a synthesis of the results of an extensive UBVI photometric study performed on a group of 14 fields located in the third quadrant of our galaxy; aimed at establishing the properties of its stellar population and the degree of agreement with two of the most important theoretical models of the Milky Way: Besançon and TRILEGAL. The individual properties of the observed stars in each field were derived by applying a software developed in-house which allows user input and condenses well established techniques of astrophysical analysis. FULL TEXT IN SPANISH

Observación versus modelos en el Tercer Cuadrante Galáctico

CARRARO, GIOVANNI;
2013

Abstract

We present a synthesis of the results of an extensive UBVI photometric study performed on a group of 14 fields located in the third quadrant of our galaxy; aimed at establishing the properties of its stellar population and the degree of agreement with two of the most important theoretical models of the Milky Way: Besançon and TRILEGAL. The individual properties of the observed stars in each field were derived by applying a software developed in-house which allows user input and condenses well established techniques of astrophysical analysis. FULL TEXT IN SPANISH
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/3213108
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