Circumstellar Material in Type Ia Supernovae via Sodium Absorption Features
Type Ia supernovae are key tools for measuring distances on a cosmic scale. They are generally thought to be the thermonuclear explosion of an accreting white dwarf in a close binary system. The nature of the mass donor is still uncertain. In the single-degenerate model it is a main-sequence star or an evolved star, whereas in the double-degenerate
Sternberg, A. et al.
Fecha de publicación:
8
2011