Not exact matches
Matter falling from a companion
star onto a
white dwarf might have induced a thermonuclear chain reaction that forced the
dwarf to expand radically without
exploding into a more common nova, Bond notes.
But it turns out
white dwarfs can breach that tipping point in another situation: Instead of a giant
star losing material to a
white dwarf, two
white dwarfs orbiting each other could slam together and
explode.
Another, less common kind of supernova, type 1a, occurs when a remnant of a
star called a
white dwarf steals matter from a companion
star until the
white dwarf explodes (SN: 4/30/16, p. 20).
At first glance this
exploding star had all the features of a type Ia supernova, which happens when a small, dense
white dwarf star steals material from an orbiting companion and then
explodes.
Sandage's preferred method is to use type Ia supernovae, which arise when a
white dwarf star gathers material from a companion and
explodes.
These so - called supersoft sources are now thought to be
white dwarf stars that cannibalize their stellar companions and then, in many cases,
explode
Astronomers believe that Type Ia supernovae occur when matter falls into an old
white -
dwarf star and pushes its mass over a threshold at which the carbon core ignites and triggers the
star to
explode.
The UCSB - led research implies that the
white dwarf was stealing matter from a much larger companion
star — approximately 20 times the radius of the sun — which caused the
white dwarf to
explode.
The
white dwarf accretes material from the companion
star, then at some point, it might
explode as a type Ia supernova.
The most famous supernovae are the result of a massive
star exploding, but a
white dwarf, the remnant of an intermediate mass
star like our Sun, can also
explode.
At the age of 20, when most college sophomores are still picking their majors, Harvard student Subrahmanyan Chandrasekhar proved that
white dwarf stars would
explode after reaching a mass 1.4 times that of our sun.
My research concentrates on the study of
exploding stars — mainly nova outbursts caused by thermonuclear explosions on the surface of
white dwarfs in binary
star systems.
As the
white dwarf accretes material from the nearby
star, it's possible that could
explode as a type la supernova.
If the
white dwarf accretes enough material to reach the Chandrasekhar limit, the maximum mass of a stable
white dwarf star (1.4 solar mass), it will likely
explode as a Type Ia supernova.