The influences of pressure ionization through radiative opacities on solar evolution models.

Details The influences of pressure ionization through radiative opacities on solar evolution models. The influences of pressure ionization through radiative opacities on solar evolution models.

Mar 1994

adsabs.harvard.edu/abs/1994ppmto..13...80l

Publ. Purple Mt. Obs., Vol. 13, No. 1, p. 80

Physics

Stellar Evolution: Solar Models

Scientific paper

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