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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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