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Fig. 8

image

A(C) vs. [Fe/H] for known CEMP stars (from Spite et al. 2013). SDSS J0222–0313 (red star) is compared to the CEMP sample stars (open red bullets) analysed in our collaboration (Bonifacio et al. 2015, 2018, 2009; Caffau et al. 2016, 2013; Sivarani et al. 2006, 2004; Spite et al. 2013; Behara et al. 2010) and unevolved CEMP stars (light blue square) and evolved CEMP stars (double light blue squares) from the literature (Yong et al. 2013; Cohen et al. 2003, 2013; Carollo et al. 2014; Masseron et al. 2012; Jonsell et al. 2006; Thompson et al. 2008; Hansen et al. 2015, 2016b; Lucatello et al. 2003; Aoki et al. 2002, 2006, 2008; Frebel et al. 2005, 2015; Li et al. 2015; Norris et al. 2007; Christlieb et al. 2004; Keller et al. 2014; Roederer et al. 2014; Ivans et al. 2005).

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