Turkish Journal of Physics
Abstract
We studied the static mass-radius relation of white dwarf stars with masses greater than 0.45 $M_\odot$. We assumed pure degenerate helium interiors at a finite temperature with luminosity-mass ratio due to neutrino energy loss. We compared the obtained M-R relation with those of other writers.
DOI
-
First Page
1
Last Page
4
Recommended Citation
CİVELEK, R, & KIZILOĞLU, N (2000). Mass-radius Relations for Helium White Dwarfs. Turkish Journal of Physics 24 (1): 1-4. https://doi.org/-
