A Statistical Discussion of Sets of Precise Astronomical by Edwin Bidwell Wilson

By Edwin Bidwell Wilson

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C 63, 032801 (2001) O. , Phys. Rev. Lett. C. , Phys. Rev. L. , Phys. Rev. W. E. H. E. Ormand, Phys. Rev. Lett. E. J. Dean and K. Langanke, Phys. Rep. 278 (1997) 1 J. Hubbard, Phys. Lett. D. Stratonovich, Sov. Phys. - Dokl. 2 (1958) 416 K. , Phys. Rev. Lett. 90 (2003) 241102 K. , Phys Rev. C67 (2003) 044314 K. J. Dean and W. Nazarewicz, Nucl. Phys. A728 (2003) 109 K. J. Dean and W. Nazarewicz, Nucl. Phys. A757 (2005) 360 K. Langanke and G. Martinez-Pinedo, Rev. Mod. Phys. W. , Phys. Rev. Lett. 91 (2003) 201102 Nuclear Astrophysics 75.

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1 Who Discovered Neutron Stars? It is well known that Baade and Zwicky hypothesized, in 1933, the existence of neutron stars as remnant cores of stars that explode as supernovae and they did so only one year after the neutron itself was discovered by Chadwick and only two years after Chandrasekhar published an analysis of the limiting mass for white dwarf (WD) stars. Contributing to this fast pace of events were the models for neutron stars by Oppenheimer and his colleagues in the late 1930s that incorporated General Relativity.

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