EDP Sciences
Free Access
Issue
A&A
Volume 509, January 2010
Article Number A93
Number of page(s) 28
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361/200911744
Published online 22 January 2010

Online Material

Table 1:  Abundances of light elements in carbon-enhanced metal-poor stars from literature. Columns (4), (6), (8), (10), (12), (15) list random errors (when available). Column (3) lists metallicities preferentially from Fe I. Column (5) list C abundances from preferencially CH determinations. (7) N abundances preferentially from CN. (9) For oxygen abundances (2) stands for measurements from O I triplet and (3) from OH lines. By default, the oxygen measurement comes from the [OI] line at 6300 Å. (11) Non-LTE corrections of O I triplet measurement according to Takeda (2003) (when applicable).

Table 2:   Abundances of neutron-capture elements in carbon enhanced metal-poor stars from literature. Columns (17), (19), (21), (23), (25) list random errors (when available). (27) Solar abundances reference adopted in the original reference source: Anders & Grevesse (1989, An89), Grevesse et al. (1996, Gr96), Grevesse & Sauval (1998, Gr98), Grevesse et al. (2000, Gr20), Asplund (2005, As05). references: (1) Cohen et al. (2004), (2) Cohen et al. (2006), (3) Lucatello et al. (2003), (4) Aoki et al. (2007), (5) Barklem et al. (2005), (6) Lucatello (2003), (7) Christlieb et al. (2002), (8) Christlieb et al. (2004), (9) Jonsell et al. (2006), (10) Norris et al. (2007), (11) Cohen et al. (2008), (12) Goswami et al. (2006), (13) Frebel et al. (2007), (14) Frebel et al. (2005), (15) Aoki et al. (2006), (16) Frebel et al. (2006), (17) Cohen et al. (2003), (18) Johnson & Bolte (2002), (19) Tsangarides (2005), (20) Aoki et al. (2002c), (21) Aoki et al. (2002d), (22) Aoki et al. (2002b), (23) Preston & Sneden (2001), (24) Sneden et al. (2003a), (25) Cayrel et al. (2004), (26) Spite et al. (2005), (27) Spite et al. (2006), (28) Barbuy et al. (2005), (29) François et al. (2007), (30) Depagne et al. (2002), (31) Sneden et al. (2003b), (32) Norris et al. (1997), (33) Bonifacio et al. (1998), (34) Aoki et al. (2002a), (35) Sivarani et al. (2006), (36) Sivarani et al. (2004), (37) Ivans et al. (2005), (38) Aoki et al. (2004), (39) Johnson & Bolte (2004), (40) Zacs et al. (1998), (41) Aoki et al. (2001), (43) Plez & Cohen (2005), (44) Deroo et al. (2005), (45) Honda et al. (2004), (46) Allen & Barbuy (2006a), (47) Christlieb et al. (2004), (48) Hill et al. (2002), (49) Plez et al. (2004), (50) Honda et al. (2006), (51) Roederer et al. (2008), (52) Paper II.

Table 3:   Same as Table 1 for stars with [C/Fe]<0.9.

Table 4:   Same as Table 2 for stars with [C/Fe]<0.9.

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