Detailed abundances from integrated-light spectroscopy: Milky Way globular clusters

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Volume 601 (May 2017)

A&A, 601 (2017) A96

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Table B.3

Abundance measurements based on theoretical isochrones.

	NGC 104	NGC 362	NGC 6254	NGC 6388	NGC 6752	NGC 7078	NGC 7099

[Fe/H]	−0.864	−1.170	−1.623	−0.710	−1.797	−2.417	−2.350
rms_w (N)	0.039 (9)	0.044 (9)	0.028 (9)	0.044 (9)	0.038 (9)	0.041 (9)	0.069 (9)
[Na/Fe]	0.426	−0.018	0.012	0.403	0.287	0.175	0.219
rms_w (N)	0.009 (2)	0.013 (2)	0.008 (2)	0.025 (2)	0.042 (2)	... (1)	0.002 (2)
[Mg/Fe]	0.436	0.190	0.370	0.164	0.369	0.177	0.264
rms_w (N)	0.095 (5)	0.088 (5)	0.082 (5)	0.107 (5)	0.120 (5)	0.115 (5)	0.147 (5)
[Ca/Fe]	0.375	0.207	0.344	0.207	0.361	0.322	0.296
rms_w (N)	0.104 (7)	0.136 (8)	0.154 (8)	0.196 (7)	0.105 (8)	0.080 (8)	0.081 (8)
[Sc/Fe]	0.230	0.135	0.176	0.105	0.040	0.243	0.138
rms_w (N)	0.148 (6)	0.054 (6)	0.093 (6)	0.143 (6)	0.067 (6)	0.096 (6)	0.103 (6)
[Ti/Fe]	0.369	0.328	0.392	0.255	0.316	0.409	0.341
rms_w (N)	0.115 (8)	0.057 (9)	0.105 (9)	0.088 (8)	0.092 (8)	0.113 (9)	0.061 (9)
[Cr/Fe]	−0.067	−0.050	0.077	−0.041	−0.089	−0.183	−0.130
rms_w (N)	0.132 (6)	0.101 (6)	0.399 (6)	0.196 (6)	0.068 (6)	0.071 (6)	0.143 (6)
[Mn/Fe]	−0.218	−0.373	−0.419	−0.131	−0.354	−0.337	−0.346
rms_w (N)	0.068 (2)	0.024 (2)	0.123 (2)	0.112 (2)	0.039 (2)	0.094 (2)	0.026 (2)
[Ba/Fe]	0.178	0.376	0.367	0.193	0.150	0.438	−0.014
rms_w (N)	0.094 (4)	0.043 (4)	0.099 (4)	0.228 (4)	0.096 (4)	0.070 (4)	0.153 (4)

Notes. For each abundance ratio, the second line lists the weighted rms and the number of individual measurements.

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