Table 2
Abundance data for the CEMP-no stars grouped in bins of iron metallicity.
Star | Teff | log ɡ | [Fe/H] | A(C) | A(Li) | 12C/13C | [Sr/Fe] | [Ba/Fe] | Source |
---|---|---|---|---|---|---|---|---|---|
MMP | |||||||||
SMSS J0313-6708 | 5125 | 2.3 | <−7.1 | 6.06 | 0.7±0.15 | 98.5±5.5 | 1,4 | ||
SMSS J1605-1443 | 4850 | 2.0 | −6.21 | 6.81 | <0.0 | 67.3±1.0 | <0.18 | <0.6 | 1, 6, 19 |
HMP | |||||||||
HE 1327-2326 | 6180 | 3.7 | −5.76 | 6.96 | <0.62 | >47 | +1.04 | 1.3 ±0.2 | 1, 2, 12 |
HE 0107-5240 | 5100 | 2.2 | −5.56 | 6.75 | <0.50 | 87.0±6 | < −0.76 | <0.2 | 2, 5, 12 |
SDSS J0023+0307 | 6140 | 4.8 | <−5.5 | 6.20 | +2.02±0.08 | 17, 21 | |||
SDSS J0815+4729 | 6050 | 4.6 | −5.50 | 7.43 | <1.3 | − | <1.02 | <1.91 | 18, 23 |
SDSS J1035+0641 | 6262 | 4.0 | <−5.2 | 7.02 | +1.90 | − | 13 | ||
SDSS J1313-0019 | 5200 | 2.6 | −5.0 | 6.42 | <0.8 | 39.1±0.6 | <−0.28 | <0.22 | 1, 15, 20 |
UMP | |||||||||
SDSS J0929+0238 | 5894 | 4.5 | −4.97 | 7.44 | - | - | <0.70 | <1.46 | 16 |
HE0557-4840 | 4900 | 2.2 | −4.81 | 5.35 | - | - | <0.0 | <−1.0 | 12 |
SDSS J1742+2531 | 6345 | 4.0 | −4.80 | 7.26 | <1.8 | - | <0.72 | <1.56 | 14 |
HE 0233-0343 | 6230 | 4.43 | −4.70 | 7.24 | +1.65±0.2 | 78.9±5.4 | +0.3 | <0.8 | 1, 7 |
SDSS J1442-0015 | 5850 | 4.0 | −4.37 | 6.02 | <1.58 | - | 13 | ||
HE1310–0536 | 5000 | 1.9 | −4.20 | 6.62 | <0.8 | 3 | −1.08±0.14 | −0.50±0.15 | 7 |
HE0057-5959 | 5257 | 2.65 | −4.08 | 5.24 | - | >2 | −0.46 | 12 | |
SDSS J0140+2344 | 5703 | 4.68 | −4.05 | 5.76 | +1.86 | >2 | +1.09 | <0.34 | 12,13 |
G77-61 | 4000 | 5.05 | −4.03 | 7.01 | <1.0 | 5+1 | <1.0 | 2, 3 | |
HE2139-5432 | 5416 | 3.04 | −4.02 | 7.03 | - | >15 | <−0.33 | 12 | |
SDSS J1034+0701 | 6224 | 4.0 | −4.01 | 6.28 | +2.24 | - | 13 | ||
SDSS J1247-0341 | 6224 | 4.0 | −4.01 | 6.64 | +2.2: | - | 13 | ||
HE0134–1519 | 5500 | 3.2 | −4.00 | 5.46 | − | >4 | −0.30±0.19 | <−0.50 | 7 |
EMP | |||||||||
CS 22949-037 | 4958 | 1.84 | −3.97 | 5.55 | <0.13 | 4+1 | +0.55 | −0.52 | 3,12 |
HE1201-1512 | 5725 | 4.67 | −3.89 | 5.94 | - | >20 | <−0.34 | 12 | |
HE1300+0157 | 5529 | 3.25 | −3.75 | 6.02 | +1.0±0.09 | >3 | <−0.85 | 12, 2 | |
HE2331–7155 | 4900 | 1.5 | −3.70 | 6.10 | − | 5 | −0.85±0.20 | −0.90±0.21 | 7 |
BD+44 493 | 5510 | 3.70 | −3.68 | 6.09 | +0.64 | - | −0.60 | 12 | |
CS 22885-096 | 5050 | 1.9 | −3.66 | 5.40 | <0.5 | - | −1.64 | 2 | |
SDSS J1349+1407 | 6112 | 4.0 | −3.60 | 6.82 | <0.9 | - | 13 | ||
HE1506-0113 | 5016 | 2.01 | −3.54 | 6.39 | +1.01±0.09 | >20 | −0.80 | 12 | |
Segue 1-7 | 4960 | 1.90 | −3.52 | 7.24 | - | >50 | 12 | ||
CS 29498-043 | 4639 | 1.00 | −3.49 | 6.87 | - | 6±2 | 2, 12 | ||
HE0146-1548 | 4636 | 0.99 | −3.46 | 6.08 | - | 4 | −0.71 | 12 | |
HE1150-0428 | 5208 | 2.54 | −3.47 | 7.36 | - | 4 | −0.54±0.14 | 2,12 | |
CS 30322-023 | 4100 | 0.3 | −3.39 | 5.87 | - | 4 | 2,3 | ||
BS 16929-005 | 5229 | 2.61 | −3.34 | 6.11 | − | >7 | −0.41 | 12 | |
CS 22957-027 | 5170 | 2.45 | −3.19 | 7.54 | − | 8±2 | −1.23±0.21 | 9,10,8 | |
LAMOSTJ1410-0555 | 6169 | 4.21 | −3.19 | 6.80 | +2.17 | −0.10 | −0.33 | 22 | |
HE1419-1324 | 4900 | 1.80 | −3.05 | 7.17 | − | 12±2 | +0.88±0.1 | 2,3 | |
SDSS J1424+5615 | 6088 | 4.34 | −3.01 | 6.94 | +2.14 | - | −0.40 | <−0.69 | 22 |
HE0100–1622 | 5400 | 3.0 | −2.90 | 8.31 | <1.12 | 13 | +0.25±0.25 | <−1.80 | 7 |
MP | |||||||||
CS 29502-092 | 5074 | 2.21 | −2.99 | 6.43 | <1.2 | 20 | −1.36+0.07 | 12, 2 | |
HE2247-7400 | 4929 | 1.56 | −2.87 | 6.29 | - | - | −0.94 | 12 | |
CS 22958-042 | 6250 | 3.5 | −2.85 | 8.76 | <0.6 | 9±2 | −0.53+0.16 | 2,3, 11 | |
CS 30314-067 | 4400 | 0.7 | −2.85 | 6.11 | <0.6 | - | −0.25 | 2 | |
CS 31080-095 | 6050 | 4.5 | −2.85 | 8.30 | +1.73±0.05 | >40 | 2,3,11 | ||
CS 22877-001 | 5100 | 2.2 | −2.72 | 6.74 | <1.2 | >10 | −0.51 | 2,3,8 | |
HE2319-5228 | 4900 | 1.6 | −2.60 | 7.56 | - | 5 | 7 | ||
CS 22945-017 | 6400 | 3.80 | −2.52 | 8.22 | - | 6±3 | 0.55±0.2 | 2,3 | |
HE1410+0213 | 4890 | 2.00 | −2.52 | 8.27 | − | 3±0.5 | +0.05±0.20 | 3 | |
CS 22956-028 | 6700 | 3.50 | −.33 | 7.97 | - | 5±2 | +0.16±0.2 | 3 | |
CS 22887-048 | 6500 | 3.7 | −1.75 | 8.17 | - | 3 | 8 |
Notes. Mega metal-poor (MMP) stars with [Fe/H] < −6.0, hyper metal-poor (HMP) stars with [Fe/H] < −5.0, ultra metal-poor (UMP) stars with [Fe/H] < −4.0, extremely metal-poor (EMP) stars with [Fe/H] < −3.0, and metal-poor (MP) stars with [Fe/H] < −1.5. The table lists the CEMP-no stars presently known for which either the carbon isotopic ratio or the Li has been measured in the literature. In boldface are the new measurements presented in this paper. Limits are at the 3σ CL.
References. 1. This paper; 2. Allen et al. (2012); 3. Masseron et al. (2010); 4. Keller et al. (2014), 5. Aguado et al. (2022), 6. Aguado et al. (2023), 7. Hansen et al. (2015), 8. Aoki et al. (2002), 9. Bonifacio et al. (1998), 10. Norris et al. (1997), 11. Sivarani et al. (2006), 12. Norris et al. (2013a), 13. Bonifacio et al. (2018), 14. Bonifacio et al. (2015), 15. Allende Prieto et al. (2015), 16. Caffau et al. (2016), 17. Aguado et al. (2019), 18. Aguado et al. (2018), 19. Nordlander et al. (2019), 20. Frebel et al. (2015), 21. Frebel et al. (2019), 22. Matsuno et al. (2017), 23. González Hernández et al. (2020).
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