STAR NO FURTHER A MYSTERY

star No Further a Mystery

A large portion of the star's angular momentum is dissipated as a result of mass loss in the stellar wind.[166] Despite this, the speed of rotation for a pulsar can be extremely fast. The pulsar at the center of the Crab nebula, as an example, rotates thirty occasions for each 2nd.[167] The rotation amount of the pulsar will gradually sluggish a re

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