Image Details
Caption: Fig. 1.
Function W(r) for solar envelope models constructed with different equations of state, heavy‐element mixtures, and abundances, as marked in the figure. All these models have their convection zone base at ﹩r_{b}=0.7133﹩ R⊙, and have a hydrogen abundance ﹩X=0.739﹩.
Other Images in This Article
Copyright and Terms & Conditions
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
Copyright ©
2025 Astronomy Image Explorer. All Rights Reserved.
