The death of a star results in a neutron star | vedclass

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(B) The evolution of a star depends on its initial mass. Stars with an initial mass roughly between $1.4M$ (the Chandrasekhar limit) and about $3M$ (t

Vedclass · Accepted Answer

Between $2M$ and $4M$

Vedclass · Answer

(B) The evolution of a star depends on its initial mass. Stars with an initial mass roughly between $1.4M$ (the Chandrasekhar limit) and about $3M$ (the Tolman-Oppenheimer-Volkoff limit) typically end their lives as neutron stars after a supernova explosion. Among the given options,the range $2M$ to $4M$ is the most appropriate representation for the progenitor mass of a neutron star. Therefore,option $B$ is correct.

The death of a star results in a neutron star if the original mass of the star in terms of the mass of the Sun $(M)$ is:

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