The first measurements of carbon isotopic ratios in post-RGB stars: SZ Mon and DF Cyg
Dusty post-red giant branch (post-RGB) stars are low- and intermediate-mass stars where the RGB evolution was prematurely terminated by a poorly understood binary interaction. These binary stars are considered to be low-luminosity analogues of post-asymptotic giant branch (post-AGB) binary stars. In this study, we investigated the chemical
Mohorian, Maksym et al.
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2024