TY  - GEN 
AU  - Salaris, M.
AU  - Domínguez Aguilera, Inmaculada
AU  - García-Berro, E.
AU  - Hernanz, M.
AU  - Isern, Jordi
AU  - Mochkovitch, R.
PY  - 1997
SN  - 0004-637X
SN  - 1538-4357
UR  - http://hdl.handle.net/10481/29067
AB  - White dwarfs are the remnants of stars of low and intermediate masses on the main sequence. Since they have exhausted all of their nuclear fuel, their evolution is just a gravothermal process. The release of energy only depends on the detailed...
LA  - eng
PB  - American Astronomical Society; Institute of Physics (IOP)
KW  - Nuclear reactions
KW  - Nucleosynthesis
KW  - Abundances
KW  - Stars interiors
KW  - White dwarf
TI  - The cooling of CO white dwarfs: influence of the internal chemical distribution
ER  -