The mechanism of Supernova Ia explosion in elliptical galaxies

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

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6 pages, 1 figure, accepted in New Astronomy

Scientific paper

10.1016/j.newast.2010.09.001

Recent observational data on the type Ia supernova rates are in excellent
agreement with the old prediction of the population synthesis of binary stars
and confirm that the overwhelming majority of type Ia supernovas (~99%) in
elliptical galaxies form via mergers of binary white dwarfs with the total mass
exceeding the Chandrasekhar limit.

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