Volume 553, May 2013
|Number of page(s)||20|
|Section||Galactic structure, stellar clusters and populations|
|Published online||30 April 2013|
Star ID, effective temperature, surface gravity, model metallicity, microturbulence, radial velocity, abundances derived from Fe I and Fe II lines, Na, and O abundances and their associated root mean square error (rms) for each of the M 15 stars analysed here as determined in C09.
Chemical abundances, uncertainties and number of lines measured here for the sample of 63 M 15 giant stars. The C09 stellar parameters, ξW13 and measured S/N are also listed.
© ESO, 2013
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