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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| Format: | Others |
| Language: | English |
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2018
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| Online Access: | http://hdl.handle.net/10183/181005 |