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

  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},
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… 


IAU Colloq. 68: Astrophysical Parameters for Globular
  • 1981
PASA, 33, e028. Bovy
  • 2015
PASA, 33, e028. Bovy
  • 2005
Visible and Near Infrared
  • 1972
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