Context. In many astrophysical contexts, the helium content of stars may differ significantly from those usually assumed in evolutionary calculations.

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Cite This Study

Bertelli et al. (Tue,) studied this question.

synapsesocial.com/papers/6a10ddb049545a83bbee86d6 https://doi.org/https://doi.org/10.1051/0004-6361:20079165

Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1Electrical and thermal conductivities of dense matter in the liquid metal phase. I - High-temperature results1983 · 203 citations
2Thermal Conduction by Electrons in Stellar Matter1969 · 249 citations
3Theoretical growth rates, periods, and pulsation constants for long-period variables1982 · 131 citations
4The equation of state for stellar envelopes. III - Thermodynamic quantities1988 · 238 citations
5A model for globular cluster extreme anomalies2007 · 110 citations

Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1Electrical and thermal conductivities of dense matter in the liquid metal phase. I - High-temperature results1983 · 203 citations
2Thermal Conduction by Electrons in Stellar Matter1969 · 249 citations
3Theoretical growth rates, periods, and pulsation constants for long-period variables1982 · 131 citations
4The equation of state for stellar envelopes. III - Thermodynamic quantities1988 · 238 citations
5A model for globular cluster extreme anomalies2007 · 110 citations