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Evidence against Anomalous Compositions for Giants in the Galactic Nuclear Star Cluster

  • Authors: B. Thorsbro, N. Ryde, M. Schultheis, H. Hartman, R. M. Rich, M. Lomaeva, L. Origlia, and H. Jönsson

2018 The Astrophysical Journal 866 52.

  • Provider: AAS Journals

Caption: Figure 1.

Six M giant stars plotted together with increasing temperature from top to bottom with blue vertical lines identifying lines of interest. The normalized fluxes have been translated upward with integer values for presentation. The stars are a mix of three Galactic center stars (GC 7688, GC 11025, and GC 11473) and three solar neighborhood stars (2M18103303–1626220, 2M18550791+4754062, and 2M21533239+5804499). The spectra show striking strong scandium, vanadium, and yttrium lines in the cooler stars, even though the stars are located in widely different environments. As temperatures increase to 3900 K and beyond, the neutral lines of scandium, vanadium, and yttrium begin to vanish, presumably due to ionization.

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