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The Chandrasekhar limit: Why only some stars become supernovas

Submit on Wednesday, May 11th, 2022 17:59

The Chandrasekhar limit determines whether a star ends its life as a smoldering white dwarf or explodes in a supernova becoming a neutron star or black hole.

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This entry was posted on Wednesday, May 11th, 2022 at 5:59 pm and is filed under NEWS. You can follow any responses to this entry through the RSS 2.0 feed. You can leave a response, or trackback from your own site.

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