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The Initial Mass Function and Other Stellar Properties Across the Core of the Hydra I Cluster

  • Authors: Ilaria Lonoce, W. L. Freedman, A. Feldmeier-Krause

Ilaria Lonoce et al 2023 The Astrophysical Journal 948 .

  • Provider: AAS Journals

Caption: Figure 14.

[α/Fe] trend when averaging: C–O (orange), Mg–Si (blue), and Ca–Ti (red). The left panel shows these as a function of the distance from NGC3309, and the right panel as a function of the velocity dispersion. Error bars in the left panel are the standard deviations of each average; to make the trends more visually clear, error bars are omitted in the right panel.

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