The Physics of Supernovae Inma Domínguez Universidad de Granada Santiago de Chile, octubre de 2007.
Type Ia Supernovae Progenitors. Type Ia Supernovae Historical defining characteristics: Generally, lack of lines of hydrogen Contain a strong Si II absorption.
Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.
OrganoSilicon Compounds Peter H.M. Budzelaar. OrganoSilicon Compounds 2 Organosilicon compounds Silicon is just like carbon, but: Larger –five- and six-coordinate.
(Informal) workshop - Ferrara April 2004 SNe. Astrophysical (natural) Explosive Devices Thermonuclear SNe Gravitational collapse C-deflagration He-detonation.
Supernovae Oscar Straniero INAF – Oss. Astr. di Collurania (TE)
