Synopsis
The Chandrasekhar limit determines whether a star ends its life as a smoldering white dwarf, or explodes in a supernova to become a neutron star or black hole.
Comments
Please to post a comment.
The Chandrasekhar limit determines whether a star ends its life as a smoldering white dwarf, or explodes in a supernova to become a neutron star or black hole.
Available in HD • 0h 3m
No comments yet. Be the first to comment.