Institute of Astronomy, Cambridge
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https://www.ast.cam.ac.uk/
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RAS Journals
@rasjournals.bsky.social
· Jul 9
Predicting metallicities and carbon abundances from Gaia XP spectra for (carbon-enhanced) metal-poor stars
ABSTRACT. Carbon-rich (C-rich) stars can be found at all metallicities and evolutionary stages. They are often the result of mass transfer from a companion
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