A Calculation of a White Dwarf Supernova

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

A hydrodynamic calculation of a 1.42M&sun; white dwarf supernova is
described. Instability and collapse are initiated by electron capture
and the subsequent nuclear detonation of C12 at high
densities is sufficient to disperse all the material of the star with an
average velocity of 7000 km/sec

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