Not exact matches
Metals (elements heavier than hydrogen and helium) are created in the interiors of stars
as they
evolve and then released into surrounding gas through
supernova explosions or stellar winds (often referred to
as chemical evolution).
As a star
evolves it produces increasingly heavy elements, and by the time it reaches
supernova status, the star is producing iron, the heaviest element possible for it to make.
«It could be created by a superluminous
supernova or a long gamma ray burst, and then later on,
as it
evolves and its rotation slows down a bit, it produces these fast radio bursts
as well
as continuous radio emission powered by that spindown.
«And each day,
as the
supernova got stronger, the lines [in the spectrum]
evolved.
Before 1987, astronomers believed that only red supergiants would explode
as supernovae, but this observation proved that other types of
evolved stars can produce these explosions too.
The violent outflowing winds
as seen in Eta Carinae herald the end of a star's life
as a
supernova, and their study provides scientists with clues about how such stars
evolve and die.
According to current theory, two different mechanisms produce
supernovae: First, stars considerably more massive than our Sun can most probably not
evolve quietly into an end state
as a white dwarf.
Both would have been born from massive stars that
evolved in close proximity in ancient star factories
as a binary pair, eventually dying
as supernovas.
Such large and luminous massive stars are believed to be highly
evolved, all of which suggests that W26 is coming towards the end of its life and will eventually explode
as a
supernova.