As a neutron star spins, its polar fountains turn with it, like an interstellar lighthouse beam.
Not exact matches
It was developed
as a testbed to validate NASA's
Neutron - star Interior Composition Explorer, or NICER, which primarily will study neutron stars and their rapidly spinning next - of - kin, pulsars, when it launches as an attached space station payload i
Neutron -
star Interior Composition Explorer, or NICER, which primarily will study
neutron stars and their rapidly spinning next - of - kin, pulsars, when it launches as an attached space station payload i
neutron stars and their rapidly
spinning next - of - kin, pulsars, when it launches
as an attached space station payload in 2017.
As gas spirals toward the
neutron star, it
spins faster and faster until some unknown trigger produces powerful, coherent radio beacons.
If the
neutron star begins life
as an X-ray binary, however, the matter accumulating on its surface causes the
neutron star to «
spin up,» increasing its rate of rotation until it
spins hundreds of times each second.
The double pulsar PSR J0737 — 3039A / B consists of two
neutron stars in a highly relativistic orbit that displays a roughly 30 - second eclipse when pulsar A passes behind pulsar B. Describing this eclipse of pulsar A
as due to absorption occurring in the magnetosphere of pulsar B, we successfully used a simple geometric model to characterize the observed changing eclipse morphology and to measure the relativistic precession of pulsar B's
spin axis around the total orbital angular momentum.
Pulsars, the dense
spinning remnants of exploded
stars, contain about the same mass
as the sun crushed into a wad of
neutrons less than 10 miles wide.
Soon after, pulsars were identified
as rapidly
spinning neutron stars, the remnants of supernova explosions; they weigh
as much
as the sun but are just a dozen miles wide.
As the
neutron star shrinks, it
spins even faster, eventually causing small fragments to detach and fly off.
Since pulsars are superdense,
spinning neutron stars left over when a massive
star explodes
as a supernova, it was logical to assume that the Monogem Ring, the shell of debris from a supernova explosion, was the remnant of the blast that created the pulsar.
Scientists have long suspected that a pulsar — a rapidly
spinning, superdense
neutron star — was born when a giant
star ended its life in a cataclysmic supernova explosion observed in late summer of 1181,
as suggested by Japanese and Chinese historical records.
Pulsars are rapidly
spinning neutron stars, which can be used
as highly accurate natural clocks in space.
Astronomers have used NASA's Chandra X-ray Observatory and other similar facilities to discover a new rotating
neutron star, which is claimed to be one of the most extreme pulsars ever detected
as its
spin period is thousands of times longer than any such objects found so far.
Once the dust clears, the only thing remaining will be a very dense
star known
as a
neutron star, these can often be rapidly
spinning and are known
as pulsars.