Virial theorem, energy content, and mass-radius-relation for white dwarfs

Details Virial theorem, energy content, and mass-radius-relation for white dwarfs Virial theorem, energy content, and mass-radius-relation for white dwarfs

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....64..289k&link_type=abstract

Astronomy and Astrophysics, vol. 64, no. 1-2, Mar. 1978, p. 289-294.

Computer Science

Numerical Analysis

21

Gravitational Effects, Stellar Mass, Virial Theorem, White Dwarf Stars, Coulomb Potential, Mass Ratios, Numerical Analysis, Radii, Stellar Evolution, Stellar Luminosity

Scientific paper

A simple model for the gravitational contraction of white dwarfs is discussed using the virial theorem. In the second part of the paper numerical calculations are reported which lead to a new mass-radius-relation for finite-temperature white dwarfs and to quantitative results concerning the contribution of different forms of energy to the luminosity.

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