Image Details
Caption: Figure 9.
Comparison of photospheric elemental abundances (﹩\mathrm{log}\varepsilon (X)﹩) for the primary (gainer) and secondary (donor) components of the Algol-type binary system ET Cru. The plot shows the spectroscopically derived abundances of He, C, N, O, Mg, Al, Si, S, and Fe in both stars. Error bars represent 1σ uncertainties.
© 2026. The Author(s). Published by the American Astronomical Society.