Table 6.
[Sr/Ba] from our sample and yield predictions. Below the CEMP sub-classification based on Beers & Christlieb (2005) and Table 4.
Star/Model | [Sr/Ba] | This study |
---|---|---|
Old (new) | ||
HE 0002–1037 | −0.95 | CEMP-r/s (r/s) |
HE 0020–1741 | 1.10 | CEMP-no (no) |
HE 0039–2635 | −0.50 | CEMP-s (r/s)* |
HE 0059–6540 | −0.50 | CEMP-r/s (r/s) |
HE 0151–6007 | −1.20 | CEMP-r/s (r/s) |
HE 0221–3218 | 0.30 | MP (MP) |
HE 0253–6024 | −0.20 | CEMP-s (s) |
HE 0317–4705 | 0.70 | CEMP-r/s (s)* |
HE 2158–5134 | 0.30 | CEMP-s (s) |
HE 2258–4427 | 0.40 | CEMP-s (s) |
HE 2339–4240 | −0.35 | CEMP-s (s) |
MHD SN | −1.80 | W12a |
1.5 AGB | −0.63 | L12b |
2.0 AGB | −0.72 | L12 |
5.0 AGB | 0.26 | L12 |
CEMP-no | [Sr/Ba] > 0.75 | New classification |
CEMP-s | −0.5 < [Sr/Ba] < 0.75 | New classification |
CEMP-r/s | −1.5 < [Sr/Ba] < −0.5 | New classification |
CEMP-r | [Sr/Ba] < −1.5 | New classification |
MP | [Sr/Ba] < 0.75 & [Ba/Fe] < 0 | New classification |
Notes. “*” indicates cases where our new classification disagrees with the old one.
W12: Yields from Winteler et al. (2012)
L12: Non-Solar-scaled data from Table 3 and 4 from Lugaro et al. (2012) taken from the end of the AGB evolution.
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