The starburst-like diagram is called a pulsar map, because it shows the location of our sun relative to known pulsars. Pulsars are the rapidly spinning remains of dying stars—the leftover cores ...

The pulsar has a spin period of 33.16 milliseconds and a dispersion measure of approximately 24.93 pc/cm 3. Previous observations of M53A have found that it is a binary system with an orbital ...

Dr Bettina Posselt explains: “We find that the most important property governing the radio emission of a pulsar is its so-called spin-down power. It quantifies the energy set free by a neutron star ...

From far off, the spinning pulsar's radio emission is perceived in pulses, much as one perceives a light signal from the rotating lantern of a lighthouse. The discovery of pulsars was exciting ...

According to the study, PSR J1617−2258A is a binary MSP with a spin period of approximately 4.32 milliseconds and a dispersion measure of 66.8 pc/cm 3. The pulsar was found in NGC 6093 and is ...

"Pulsars also emit particles at very high speeds, which beams away energy. These effects lead to the pulsar spinning more slowly as time goes on, and currently there isn't any way to calculate how ...

Pulsar J1719-1438 is a very fast-spinning pulsar—what’s called a millisecond pulsar. Amazingly, it rotates more than 10,000 times per minute, has a mass of about 1.4 times that of our Sun but is only ...

Most of this radiation is in the form of X-Rays which power the compact source. There exists an offset angle between the dipole magnetic axis and the spin axis of the Pulsar. So, when radiation is ...