Not exact matches
Chemical calculations show that helium hydride should be visible
in clouds around distant galaxies and
supernovas, or even
in modern planetary nebulas (shells of gas
expelled by aged, sunlike stars).
A ring of hot spots (
in images from the Hubble Space Telescope) gradually lit up as a shock wave from
supernova 1987A plowed through a loop of gas that had been
expelled by the star tens of thousands of years before the explosion.
A shock wave from that collapse will speed outward, violently
expelling the star's outer layers
in a massive explosion known as a
supernova.
Supernovas pack a lot of punch, to put it lightly — they can outshine galaxies and
expel more energy than our Sun's lifetime output, making them the largest explosions
in space.
A new study led by Keiichi Ohnaka, a researcher at Catholic University of the North
in Chile, sought to understand how the distant red supergiant star Antares manages to
expel so much matter off its surface as it nears the end of its life and nears its finale as a spectacular
supernova.
Some are found
in globular clusters, but most move
in a huge cloud around the disk called the galactic halo, which has a luminous inner component defined by globular star clusters and other easily observable stars (with coronae of hot gas possibly
expelled by
supernovae and of high - velocity neutron stars) and an outer dark - matter component inferred from its gravitational impact on the Milky Way's spiral disk.
The outer layers rebound from the core and are
expelled into space
in a gaint
supernova explosion.