Autor:	Niem, D., Geppert, U., Wiebicke, H. -J.
Zdroj:	Astrophysics and Space Science; March 1985, Vol. 110 Issue: 2 p331-336, 6p
Abstrakt:	Motivated by the discovery of the millisecond pulsars, we consider the effect of rapid rotation on the envelope of a neutron star. Solving the equation of hydrostatic equilibrium we find expressions for the density and oblateness as functions of radius and polar angle.
Databáze:	Supplemental Index
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