Pulsars, aka spinning neutron stars, normally
emit radio pulses like clockwork.
Not exact matches
Katelin Schutz, a theorist at the University of California, Berkeley, says that clarity could come even faster from stellar beacons called millisecond pulsars, which
emit exquisitely regular
pulses of
radio waves.
In 1974, astronomers Russell Hulse and Joseph Taylor detected a binary pulsar, a pair of two dead stars
emitting pulses of
radio waves.
The nebula contains a pulsar in its centre which rotates thirty times per second,
emitting pulses of radiation from gamma rays to
radio waves.
Like turning the knob on a
radio, the team adjusted the
pulse so that, if the artificial horizon
emitted any Hawking radiation, its wavelength would be between 800 and 900 nanometers, a range that could not be confused with other sources such as laser - induced fluorescence.
Radar
pulses (short bursts of
radio - frequency energy)
emitted from a ground - based transmitter are reflected by a meteor's trail.
Although neutron stars were predicted in the 1930s, it was not until the late 1960s that observers accidentally discovered a
radio source
emitting weak
pulses, each lasting about 0.3 second with a remarkably constant period of approximately 1.337 seconds.
Pulsars are compact, rotating neutron stars that act like cosmic lighthouses and
emit regular
radio pulses whose periods can be measured very precisely.
But instead of
pulses of sound or
radio waves, a LIDAR scanner
emits laser beams and measures the time that they take to return in order to map the location and elevation of objects in the surrounding area.