Interpolations of Rosseland-mean opacities for variable X and Z
- 1 March 1996
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 279 (1) , 95-100
- https://doi.org/10.1093/mnras/279.1.95
Abstract
For fixed relative abundances of ‘metal’ atoms, stellar compositions are specified by mass fractions X for hydrogen and Z for metals (the helium mass fraction being Y=1−X−Z).Keywords
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