According to the provided table, what is the approximate initial stellar mass range that results in a Neutron Star remnant?
Answer
$8 M_{\odot}$ to $\approx 20 M_{\odot}$
The table specifies that progenitors with initial masses approximately between $8 M_{\odot}$ and $20 M_{\odot}$ result in a core remnant classified as a Neutron Star.
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