Simulations indicate that the low-mass star in the J0453+1559 binary system could be a neutron star rather than a white dwarf. The star's mass, 1.174 M ⊙ , is unusually low for a neutron star.
The gargantuan collision ... stars orbit each other in pairs, or binaries. If their orbit is tight enough, the effects of Einstein’s general theory of relativity kick in, and the binary starts ...
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