On the lower mass limit for gravitational collapse of evolved stars.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Stellar Interiors: Gravitational Collapse, Stellar Evolution: Supernovae

Scientific paper

The authors examine some aspects of the physics which determines the
ignition density for explosive Ne burning in stars in the 8
Msun ≤ M ≤ 10 Msun range and thus the lower
mass limit for gravitational collapse of single stars.

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