At higher frequencies, the intrinsic strength of the pulsar signals largely decreases as
pulsar radio emission usually has a steep spectrum.
Not exact matches
Discovered initially by lighthouse - like beams of
radio emission, more recent research has found that energetic
pulsars also produce beams of high energy gamma rays.
«We think it's quite possible that the
radio beam is narrower than the gamma - ray
emission, but we don't yet know how gamma rays are produced in the
pulsar,» says Fermi project scientist Steve Ritz of NASA's Goddard Space Flight Center in Greenbelt, Maryland.
The top candidates, the astronomers suggested, are a neutron star, possibly a highly - magnetic magnetar, surrounded by either material ejected by a supernova explosion or material ejected by a resulting
pulsar, or an active nucleus in the galaxy, with
radio emission coming from jets of material emitted from the region surrounding a supermassive black hole.
For comparison, this
pulsar's
radio emission is some 250 times weaker than that from the famous
pulsar in the Crab Nebula (the remnant of an explosion in the year 1054 recorded by Chinese astronomers and possibly also by Native Americans of the Anasazi tribe in modern - day Arizona and New Mexico).
By detecting this
pulsar in the
radio spectrum, astronomers may now follow its evolution with greater ease and flexibility than with X-ray telescopes on satellites, study the
pulsar emission mechanisms, and also characterize the dynamic interstellar medium between the Earth and the
pulsar.
We observe pulsed
radio emission, like
pulsars, but not for every rotation of the star.