Evolutionary sequences for H and He atmosphere massive white dwarf stars

White dwarf stars are the most common final stage of stellar evolution, corresponding to 99% of all stars in the Galaxy. White dwarf models can be used to obtain the age of stellar populations, to build an initial to final mass relation to understand the connection between the properties of white dw...

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Bibliographic Details
Main Author: Ramos, Gabriel Lauffer
Other Authors: Romero, Alejandra Daniela
Format: Others
Language:English
Published: 2018
Subjects:
Online Access:http://hdl.handle.net/10183/181005

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