The standard lower limit for the mass of white dwarfs (WDs) with a C/O core is roughly 0.5 Modot. In the present work we investigate the possibility to form C/O WDs with mass as low as 0.33 Modot. Both the pre-WD and the cooling evolution of such nonstandard models are described.

C/O white dwarfs of very low mass: 0.33-0.5 Mo

PRADA MORONI, PIER GIORGIO;
2009-01-01

Abstract

The standard lower limit for the mass of white dwarfs (WDs) with a C/O core is roughly 0.5 Modot. In the present work we investigate the possibility to form C/O WDs with mass as low as 0.33 Modot. Both the pre-WD and the cooling evolution of such nonstandard models are described.
2009
PRADA MORONI, PIER GIORGIO; Straniero, O.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11568/133216
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