Volume 383, Number 3, MarchI 2002
|Page(s)||L27 - L30|
|Published online||15 March 2002|
Letter to the Editor
He-detonation in sub-Chandrasekhar CO white dwarfs: A new insight into energetics and -process nucleosynthesis
Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, CP 226, 1050 Brussels, Belgium
2 Departament de Fisica i Enginyeria Nuclear, Universitat Politecnica de Catalunya, Av. Víctor Balaguer s/n, 08800 Vilanova i la Geltrú (Barcelona), Spain, and Institut d'Estudis Espacials de Catalunya, Ed. Nexus-201, C/ Gran Capità 2-4, 08034 Barcelona, Spain
3 Institut de Ciències de l'Espai, CSIC, Barcelona, Spain, and Institut d'Estudis Espacials de Catalunya, Ed. Nexus-201, C/ Gran Capità 2-4, 08034 Barcelona, Spain
Corresponding author: S. Goriely, firstname.lastname@example.org
Accepted: 13 January 2002
He-accreting white dwarfs with sub-Chandrasekhar mass are revisited. The impact of the use of an extended reaction network on the predicted energy production and characteristics of the detonating layers is studied. It is shown that the considered scenario can be the site of an -process combined with a p-process and with a variant of the rp-process we refer to as the pn-process. We define the conditions under which the derived distribution of the abundances of the p-nuclides in the ejecta, including the puzzling light Mo and Ru isotopes, mimics the solar-system one.
Key words: hydrodynamics / nuclear reactions / nucleosynthesis / shock waves / stars: white dwarfs
© ESO, 2002
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.