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This article has been cited by the following article(s):
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s-Process Enriched Evolved Binaries in the Galaxy and the Magellanic Clouds
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Dust from evolved stars: a pilot analysis of the AGB to PN transition
F Dell’Agli, S Tosi, D Kamath, L Stanghellini, S Bianchi, P Ventura, E Marini and D A García-Hernández Monthly Notices of the Royal Astronomical Society 526(4) 5386 (2023) https://doi.org/10.1093/mnras/stad3080
Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars