A large sample of newly-identified carbon-deficient red giants from APOGEE
Sunayana Maben, Yerra Bharat Kumar, Bacham E. Reddy, Simon W., Campbell, Gang Zhao

TL;DR
This study identified 103 new carbon-deficient red giants using APOGEE data, revealing their distribution across the Galaxy and their evolutionary phases, with detailed chemical composition analysis suggesting extensive hydrogen burning and varied origins.
Contribution
The paper significantly increases the known sample of carbon-deficient red giants and provides new insights into their distribution, evolutionary states, and chemical compositions.
Findings
103 new CDGs identified, tripling previous counts
CDGs are very rare, about 0.03% of giants
CDGs are found throughout all Galactic components
Abstract
Based on the APOGEE survey we conducted a search for carbon-deficient red giants (CDGs). We found 103 new CDGs, increasing the number in the literature by more than a factor of 3. CDGs are very rare, representing ~per cent of giants. They appear as an extended tail off the normal carbon distribution. We show that they are found in all components of the Galaxy, contrary to previous findings. The location of CDGs in the Hertzsprung-Russell diagram (HRD) shows that they are primarily intermediate-mass stars (). Their extended distribution may indicate that CDGs can also sometimes have . We attempted to identify the evolutionary phases of the CDGs using stellar model tracks. We found that the bulk of the CDGs are likely in the subgiant branch or red clump phase, whereas other CDGs may be in the red giant branch or early asymptotic giant…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
