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Insights into thermonuclear supernovae from the incomplete Si-burning process

Autor
Bravo, E.
Tipus d'activitat
Article en revista
Revista
Astronomy and astrophysics
Data de publicació
2013-01-21
Volum
550
Pàgina inicial
1
Pàgina final
16
DOI
https://doi.org/10.1051/0004-6361/201220309 Obrir en finestra nova
Repositori
http://hdl.handle.net/2117/17442 Obrir en finestra nova
URL
http://www.aanda.org/index.php?option=com_article&access=doi&doi=10.1051/0004-6361/201220309&Itemid=129 Obrir en finestra nova
Resum
Type Ia supernova (SNIa) explosions synthesize a few tenths to several tenths of a solar mass, whose composition is the result of incomplete silicon burning that reaches peak temperatures of 4 GK to 5 GK. The elemental abundances are sensitive to the physical conditions in the explosion, making their measurement a promising clue to uncovering the properties of the progenitor star and of the explosion itself. Using a parameterized description of the thermodynamic history of matter undergoing inco...
Citació
Bravo, E. Insights into thermonuclear supernovae from the incomplete Si-burning process. "Astronomy and astrophysics", 21 Gener 2013, vol. 550, p. 1-16.
Paraules clau
Abundances, Nuclear reactions, Nucleosynthesis, Supernovae - general, White dwarfs
Grup de recerca
GRPFM - Grup de Recerca en Propietats Físiques dels Materials

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