Massive spheres with an isothermal core

Details Massive spheres with an isothermal core Massive spheres with an isothermal core

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jpha...13.1729d&link_type=abstract

Journal of Physics A - Mathematical and General, vol. 13, May 1980, p. 1729-1736.

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3

Isothermal Processes, Neutron Stars, Stellar Mass, Stellar Models, Stellar Structure, Cores, Radii, Red Shift, Stellar Envelopes

Scientific paper

Massive spherical configurations with an isothermal core and an inverse-square variation of density in the envelope have been studied. It is found that such structures are pulsationally stable. Keeping in view the relativistic restriction on the speed of a signal, it is found that K(max) = 0.80 for such structures. The maximum surface and central red shifts are found to be 0.502 and 28.7, respectively. An application of such structures to the case of a neutron star gives the maximum mass and size of the star to be 2.31 solar masses and 12.2 km.

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