Pulsar wind nebulae (PWNe) are highly energetic and dynamic structures that form around pulsars, which are rapidly rotating neutron stars emitting beams of radiation, including X-rays and gamma rays. When a pulsar is born from the supernova explosion of a massive star, it can generate a significant outflow of charged particles, known as the pulsar wind. This wind consists mainly of electrons and positrons, and it moves outward at nearly the speed of light.
Articles by others on the same topic
There are currently no matching articles.