Matched GALAH pairs reveal sub-percent C2/CN and hydrogen line-width differences between red clump and red giant branch stars, including a microturbulence offset.
C., et al., 2010, in McLean I
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Optical spectroscopic signatures of the red giant evolutionary state
Matched GALAH pairs reveal sub-percent C2/CN and hydrogen line-width differences between red clump and red giant branch stars, including a microturbulence offset.