Previously it was
thought that supernova typically have one of two main scenarios. But a team of
astronomers, including Wendy Friedman, Mark Phillips and Eric Persson of
Carnegie, reported the discovery of a new type of supernova, called type 1ah.
Astronomers used to
divide supernova into two main categories: type 1a supernova and supernova occurring core-collapse. Supernova, accompanied by collapse of the core,
are
explosions of stars whose masses range from 10 to 100 times the mass of our
Sun. Supernovae type 1a is almost complete destruction of the tiny white dwarf.
A new type of supernova
1ah, much less bright and less powerful than the type 1a. Although the core of
both of these types is the explosion of white dwarf, but SNe 1ah not destroy it
completely.
Based on numerous
observations, the researchers concluded that SNe 1ah occur in binary systems,
which include the white dwarf and its companion - a normal star, which loses
its outer layer of hydrogen remaining enriched with helium. Helium white dwarf
pulls from the normal star, which leads to an explosion, scientists say.
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