This question comes from William.
He writes "Hi Fraser, I was wondering if you
could do a video on pulsars like you did on
quasars."
You got it.
Stars are held in perfect balance between
the pressure of gravity pulling them inward,
and the outward force of radiation.
Once stars runs out of fuel, they collapses
in on themselves - it's the amount of mass
decides what happens next.
The most massive stars detonate as supernovae,
and can explode or collapse into black holes.
If they're less massive, like our Sun, they
blast away their outer layers and then slowly
cool down as white dwarfs.
But for stars between 1.4 and 3.2 times the
mass of the Sun, they may still become supernovae,
but they just don't have enough mass to make
a black hole.
These medium mass objects end their lives
as neutron stars, and some of these can become
pulsars or magnetars.
Gravity overwhelms the atomic bonds of the
matter in a neutron star, crushing protons
and electrons together into neutrons.
This is how they get their name.
A star that used to be more than a million
kilometers wide is now less than 20 kilometers
across.
This material is so dense, that a single sugar
cube's worth weigh about 100 million tonnes
on Earth.
And you would need to be traveling 100,000
km/s to escape a neutron star's pull - about
1/3rd the speed of light.
So that's how you get a neutron star.
But what about these pulsars?
When these stars collapse, they maintain their
angular momentum.
But with a much smaller size, their rotational
speed increases dramatically, spinning many
times a second.
This relatively tiny, super dense object,
emits a powerful blast of radiation along
its magnetic field lines.
Although this beam of radiation doesn't necessarily
line up with it's axis of rotation.
And so, from here on Earth, astronomers detect
an intense beam of radio emissions several
times a second, as it rotates around like
a lighthouse beam.
This is a pulsar.
The first one was detected in 1967 by Jocelyn
Bell Burnell and Antony Hewis.
They detected a mysterious radio emission
coming from a fixed point in the sky that
peaked every 1.33 seconds.
Although they were certain it had a natural
origin, they named it LGM-1, which stands
for "little green men", and subsequent discoveries
have helped astronomers discover the true
nature of these strange objects.
Pulsars have been discovered emitting many
different wavelengths of light, from radio
to visible and even X and gamma rays.
There have been a total of 1600 found so far,
and the fastest discovered emits 716 pulses
a second.
When a pulsar first forms, it has the most
energy and fastest rotational speed.
As it releases electromagnetic power through
its beams, it gradually slows down.
Within 10 to 100 million years, it slows to
the point that its beams shut off and the
pulsar becomes quiet.
When they are active, they spin with such
uncanny regularity that they're used as timers
by astronomers.
Pulsars help us search for gravitational waves,
probe the interstellar medium, and even find
extrasolar planets in orbit.
It has even been proposed that spacecraft
could use them as beacons to help navigate
around the Solar System.
On NASA's Voyager spacecraft, there are maps
that show the direction of the Sun to 14 pulsars
in our region.
If aliens wanted to find our home planet,
they couldn't ask for a more accurate map.
I hope 
that helps, William.
