Photo-chemo-dynamical analysis and the origin of the bulge globular cluster, Palomar 6

@article{Souza2021PhotochemodynamicalAA,
  title={Photo-chemo-dynamical analysis and the origin of the bulge globular cluster, Palomar 6},
  author={Stefano O. Souza and Marica Valentini and Beatriz Barbuy and Angeles P'erez-Villegas and Cristina Chiappini and S. Ortolani and Domenico Nardiello and Bruno Dias and Friedrich Anders and E. Bica},
  journal={Astronomy \& Astrophysics},
  year={2021}
}
Context. Palomar 6 is a moderately metal-poor globular cluster projected towards the Galactic bulge. A full analysis of the cluster can give hints on the early chemical enrichment of the Galaxy and a plausible origin of the cluster. Aims. The aim of this study is threefold: a detailed analysis of high-resolution spectroscopic data obtained with the UVES spectrograph at the Very Large Telescope (VLT) at the ESO, the derivation of the age and distance of Palomar 6 from Hubble Space Telescope (HST… 

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Abundance pattern [X/Fe] vs. atomic number (Z) of the references moderately metal-poor bulge GCs NGC 6558, NGC 6522, M62, and HP 1. The colours are the same as Figure 8