Question: Question 2 ( 1 point ) Massive stars ( more than 1 0 - 1 2 solar masses ) leave their core as a spinning
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Massive stars more than solar masses leave their core as a spinning neutron star. Sometimes it can be viewed as a pulsar such as the one observed via radio in the Crab Nebula. The pulses appear every ms What is the angular frequency of the Crab Nebula pulsar in rads
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