A pulsar is a highly magnetized, rotating neutron star that emits beams of electromagnetic radiation out of its magnetic poles. The radiation is observed as pulses of light when the beam of emission is pointing towards the Earth, much like a lighthouse beam. Pulsars were first discovered in 1967 by Jocelyn Bell Burnell and Antony Hewish.
Pulsars are formed when the core of a massive star undergoes a supernova explosion and collapses into a neutron star. The conservation of angular momentum causes the neutron star to rotate rapidly, and the compression of the core leads to the generation of an intense magnetic field.
To understand pulsars better, consider studying the following topics:
By delving into these topics, you can gain a comprehensive understanding of pulsars and their place in the cosmos.
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