Volume 574, February 2015
|Number of page(s)||33|
|Published online||02 February 2015|
Atomic and molecular features used to classify C, M- and S-type stars.
74 candidate AGB sources in the inner region (≤3 kpc) for which spectra with S/N ≥ 10 were obtained.
73 candidate AGB sources in the outer region (≥ 5 kpc) for which spectra have been obtained.
43 candidate AGB sources in the inner (top) and outer (bottom) regions for which we are able to offer a tentative classification despite the low S/N of the spectra obtained.
Spectral source counterpart IDs.
© ESO, 2015
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