Table 1
Stars among the ≈1500 O-rich stars in the catalog of Messineo & Brown (2019) that are flagged as C-rich by the LPV pipeline.
| Alias | Name DR3 | Area(a) | Spec. type(b) | Inspection |
|---|---|---|---|---|
| IRC +60091 | 465401835863237504 | A | M2 Iab | |
| CD-61 3575 | 6055427493901807104 | A | M2 I | |
| IRAS 12563-6100 | 6055686944283937408 | A | M4 I-II | |
| KW Sgr | 4063462206570029312 | A | M1.5 I | |
| IRC-20409 | 4069136201903321600 | A | M3 | |
| PER085 | 523056686572432768 | B | M2 Iab | |
| HD 12014 | 507785054178237824 | B | K1 | |
| HD 115921 | 5868597894009411328 | B | K4.5 Iab-Ib | S? (Skiff’s communication) |
| IRAS 14599-5941 | 5876489879290620416 | B | M3.2Ib-II | |
| W Per | 460621159304139008 | B | M4.5 I | |
| AS 381 | 2055181605358559872 | B | K0I-II+B1[e] | emission |
| PER287 | 2198645646339039360 | B | M2 Iab | |
| PER572 | 444883608855838720 | E | M4 Ib-II | |
| MZM22 | 4146602259265301632 | E | M0 I |
Notes. A visual inspection of their BP/RP spectra does not confirm their C-rich nature. (a)Area designates a specific region of the Luminosity versus Teff diagram (Messineo & Brown 2019). In particular, area A includes stars brighter than the AGB limit.(b) Spectral types are collected from the literature by Messineo & Brown (2019).
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