The globular cluster AL~3 is old and located in the inner bulge. Three individual stars were observed with the Phoenix spectrograph at the Gemini South telescope. The wavelength region contains prominent lines of CN, OH, and CO, allowing the derivation of C, N, and O abundances of cool stars. We aim to derive C, N, O abundances of three stars in the bulge globular cluster AL3, and additionally in stars of NGC 6558 and HP1. The spectra of AL3 allows us to derive the cluster's radial velocity. For AL3, we applied a new code to analyse its colour-magnitude diagram. Synthetic spectra were computed and compared to observed spectra for the three clusters. We present a detailed identification of lines in the spectral region centred at 15555 A, covering the wavelength range 15525-15590 A. C, N, and O abundances are tentatively derived for the sample stars.
@article{arxiv.2102.12674,
title = {Gemini/Phoenix H-band analysis of the globular cluster AL3},
author = {B. Barbuy and H. Ernandes and S. O. Souza and R. Razera and T. Moura and J. Meléndez and A. Pérez-Villegas and M. Zoccali and D. Minniti and B. Dias and S. Ortolani and E. Bica},
journal= {arXiv preprint arXiv:2102.12674},
year = {2021}
}
Comments
14 pages, 13 figures, accepted for Astronomy & Astrophysics