What is the approximate upper limit on the remnant core mass for the object to stabilize as a neutron star?

Answer

Around 2 to 3 solar masses

If the remnant mass of the core left behind after the explosion remains below a critical threshold, typically estimated between 2 to 3 solar masses, it stabilizes as a neutron star.

What is the approximate upper limit on the remnant core mass for the object to stabilize as a neutron star?

#Videos

A Detailed Breakdown of Core Collapse Supernovae

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