A scale transformation is obtained which allows the Hertel and Thirring (1971) gravitational-phase-transition theory to be extended to more generalized astrophysical conditions. It is shown that by means of this transformation, the formation of core-halo structures in late-type stars can be explained. The effect of the physical conditions peculiar to this type of star is discussed.
Gravitational phase transitions and the late-type stars
PAOLICCHI, PAOLO
1977-01-01
Abstract
A scale transformation is obtained which allows the Hertel and Thirring (1971) gravitational-phase-transition theory to be extended to more generalized astrophysical conditions. It is shown that by means of this transformation, the formation of core-halo structures in late-type stars can be explained. The effect of the physical conditions peculiar to this type of star is discussed.File in questo prodotto:
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