Stellar populations and interstellar medium in nearby galaxies with MEGARA@GTC
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Publication date
2024
Defense date
12/04/2023
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Universidad Complutense de Madrid
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Abstract
La evolución de las galaxias es el resultado de una gran cantidad de interacciones muy complejas que tienen lugar entre los distintos componentes que las conforman. Esto hace que desentrañar los misterios que aún permanecen desconocidos necesite de una cantidad ingente de datos que abarquen la mayor cantidad posible de observables. El objetivo de esta tesis es profundizar en el conocimiento que tenemos sobre las características que presentan las poblaciones estelares y el medio interestelar en las galaxias cercanas ayudándonos de las últimas herramientas desarrolladas en el campo de la astrofísica...
The evolution of galaxies is the result of a large number of very complex interactions that take place between the different components that make them up. This means that unravelling the mysteries that remain unknown requires a huge amount of data covering as many observables as possible. The aim of this thesis is to deepen our knowledge of the characteristics of stellar populations and the interstellar medium in nearby galaxies with the help of the latest tools developed in the field of astrophysics...
The evolution of galaxies is the result of a large number of very complex interactions that take place between the different components that make them up. This means that unravelling the mysteries that remain unknown requires a huge amount of data covering as many observables as possible. The aim of this thesis is to deepen our knowledge of the characteristics of stellar populations and the interstellar medium in nearby galaxies with the help of the latest tools developed in the field of astrophysics...
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Tesis inédita de la Universidad Complutense de Madrid, Facultad de Ciencias Físicas, leída el 12/04/2023. Tesis formato europeo (compendio de artículos)