Astronomers know that black holes ranging from about 10 times to 100 times the mass of our sun are
the remnants of dying stars, and that supermassive black holes, more than a million times the mass of the sun, inhabit the centers of most galaxies.
Scientists have been studying
the remnants of this dying star, known as 1987A, ever since.
The donut of material confines the intense radiation coming from
the remnant of the dying star.
Not exact matches
When they
die,
stars explode in supernovae, leaving behind a cloud
of ejected material called a supernova
remnant.
Norbert Schulz and Nicola Omodei discuss the recent detection
of a
dying star igniting the most powerful blast ever seen — something so powerful it radiated energy that was 500 million times that
of visible light and how scientists have discovered that a familiar sight in the skies is actually our earliest view yet
of a
star being consumed by the
remnant of a nearby exploded
star.
A more powerful type
of X-ray source is a supernova
remnant, the gaseous shell ejected during the violent explosion
of a
dying star.
In a stellar black hole, which forms when a giant
star dies explosively, the rotation is a logical
remnant of the
star's spin.
Those
remnants are the rubble left over from the explosions
of dying stars, which in turn become incorporated into newly forming planets.
NuSTAR, a high - energy X-ray observatory, has created the first map
of radioactive material in a supernova
remnant called Cassiopeia A, or Cas A, to reveal how shock waves likely tear massive
dying stars apart, the researchers said in a study, published in the Feb. 20 issue
of Nature.
The most massive
of these
dying stars leave behind a
remnant known as a black hole.