Mass and radius of PSR J0030+0451 measured as 1.44 solar masses and 13.02 km, improving astrophysical constraints on the cold dense matter equation of state.
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Strange quark matter strangelets with low baryon number can form stable self-gravitating sub-stellar objects, predicting a new class of ultra-compact candidates with a density gap from ordinary planets and brown dwarfs.
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PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
Mass and radius of PSR J0030+0451 measured as 1.44 solar masses and 13.02 km, improving astrophysical constraints on the cold dense matter equation of state.
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Sub-stellar Strange Quark Matter Objects: Predicting a New Class of Highly-Compact Candidates
Strange quark matter strangelets with low baryon number can form stable self-gravitating sub-stellar objects, predicting a new class of ultra-compact candidates with a density gap from ordinary planets and brown dwarfs.