It is thought to have been
produced in supernova nucleosynthesis from the collision of two neutron stars and to have been present in the dust from which the Solar System formed.
The stronger moving magnetic fields
produced in supernova explosions could provide the energy for most other cosmic rays.
They are abundantly
produced in supernova explosions, star - powering nuclear fusion and other nuclear processes, resulting in trillions of neutrinos passing through us every minute.
Then, researchers led by Alexander Kusenko at the University of California in Los Angeles, US, calculated that sterile neutrinos
produced in supernova explosions could «kick» the neutron stars created in the supernovae to speeds of 1000 kilometres per second — a phenomenon that had previously been unexplained.
Those objects are
produced in supernovae, and CCCP has now found several more possible neutron stars.
Not exact matches
«Gordon Garmire, now a Penn State Evan Pugh Professor Emeritus of Astronomy and Astrophysics, discovered
in 1979 that the
supernova surrounding this object was
producing X-rays.
In the failed
supernova of a red supergiant, the envelope of the star is ejected and expands,
producing a cold, red transient source surrounding the newly formed black hole, as illustrated by the expanding shell (left to right).
The results resolve some of the questions regarding the
supernova - GRB connection, but it remains unclear how a single mechanism can
produce supernovae and the much more powerful GRBs
in the distant universe.
Two neighboring stars may have obliterated themselves
in a pair of explosions called
supernovas,
producing two black holes.
A new study reveals that neutrinos
produced in the core of a
supernova are highly localised compared to neutrinos from all other known sources.
Studies using type 1a
supernovas as «standard candles» to measure how fast the universe expands (the Hubble constant)
produce a result
in conflict with other data used to infer the cosmic growth rate.
Neutrinos are elementary particles
produced in the nuclear furnaces inside stars and
in supernova explosions.
A
supernova that went off
in 1987
produced large quantities of dust, which may explain why galaxies
in the early universe were so dusty
Antimatter flits into existence
in a variety of ways: it is
produced by black holes,
supernovas, and some types of radioactive decay.
Supernova explosions of individual stars
in our Milky Way galaxy should also
produce detectable gravitational waves, which could help astrophysicists figure out exactly how the stars blow up.
It had been thought that heavier elements are forged during
supernova explosions, but computer simulations of the process didn't always
produce the proportions of these elements seen
in nature.
Other cosmic phenomena such as
supernovae in the Milky Way and colliding neutron stars
in our galactic neighborhood should also
produce detectable gravitational waves, each with their own accompanying revolutionary insights, but so far all three of LIGO's detections have been death - rattles from merging pairs of black holes
in remote stretches of the universe.
«We are now fully confident that one of the most popular
supernova remnants detected
in our galaxy was
produced by an ordinary type Ia
supernova that was first detected more than 400 years ago,» write Andrea Pastorello of Queen's University Belfast and Ferdinando Patat of the European Southern Observatory
in Germany
in a commentary on the study.
Stars with a few to about 30 times the mass of the Sun are thought to collapse to form neutron stars,
producing a
supernova in the process.
And then I also thought about the fact that over the history of the life of the universe, neutrinos are not just
produced by the sun, but when stars explode
in a
supernova, the most brilliant fireworks
in the universe, as brilliant as those fireworks are, less than 1 percent of the energy of the star is coming out
in light; 99 percent is coming out as neutrinos and so neutrinos are being, [and] every time [a star explodes there's] an incredible burst of neutrinos.
The aftermath of the neutron star collision detected
in August included the gravitational waves spotted by LIGO and VIRGO (pale arcs); a near - light - speed jet that
produced gamma rays (magenta); expanding debris from a kilonova — an explosion similar to a
supernova, but smaller — that
produced ultraviolet (violet), optical and infrared (blue - white to red) emission; and X-rays (blue).
Some cosmic rays detected on Earth are
produced in violent events such as
supernovae, but we still don't know the origins of the highest - energy particles, which are the most energetic particles ever seen
in nature.
My research is focused on understanding the origin of «stardust»
produced in the envelopes of low - mass stars or
in supernova explosions, and preserved
in carbonaceous meteorites and interplanetary dust particles.
They are thus probably more similar to galaxies
in the early Universe when there had been less time for stars to
produce the heavy elements and then return them to their surroundings through
supernova explosions.
The second process relies on the fact that stars also contain smaller amounts of carbon
produced in previous generations of stars that exploded as
supernovas.
In any case, any developing carbon - based life on a developing Earth - type planet would be subject to tremendous heat on a newly formed planet that is under intense asteroidal and cometary bombardment, in addition to the intense and deadly radiation produced by nearby supernovae and other massive young star
In any case, any developing carbon - based life on a developing Earth - type planet would be subject to tremendous heat on a newly formed planet that is under intense asteroidal and cometary bombardment,
in addition to the intense and deadly radiation produced by nearby supernovae and other massive young star
in addition to the intense and deadly radiation
produced by nearby
supernovae and other massive young stars.
A Type Ic
supernova may be
produced by a high - mass star that has blown off much of its outer hydrogen layer while still retaining a significant helium layer, and so it is similar to a Type Ib except that helium is seen
in its spectrum.
The
supernova explosion that
produced the Crab pulsar occurred
in the year 1054 and was documented by Chinese astronomers.
HEFT will map the hard X-ray emission from
supernova remnants to investigate issues of stellar nucleosynthesis (through the mapping of radioactive Titanium) and study the origin and acceleration of cosmic - rays (through mapping the continuum hard X-rays
produced in the same shocks that
produce the cosmic - rays).
Indeed, GRBs appear to emit
produce even more energy than
supernovae or even quasars (which are energetically bright accretion disks and bi-polar jets around supermassive black holes that are most commonly found
in the active nuclei of some distant galaxies and possibly even
in the pre-galaxy period after the Big Bang).
The next step would be to look for presence of Lithium - 7 and Boron - 11 — also
produced by neutrino spallation
in supernovae —
in meteorites.
While other objects
in the universe generate cosmic rays, most probably active galactic nuclei located far beyond our own Milky Way galaxy,
supernovae in our own galactic neighborhood are thought to
produce a large fraction of the cosmic rays that impact Earth.
This first is a black tape installation around the entirety of the wall space
in the Main Gallery derived from the atomic radii of the elements
produced in suns that are large enough to complete their life cycles as
supernovas.
So would past variations
in our local star — or a long - ago local
supernova —
produced a pulse of warming?