Image Details

Choose export citation format:

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 11.

Correlations between IMF slope and velocity dispersion (left), and metallicity (right). Points are color-coded as in Figure 6, with darker red in the center. Diamonds refer to NGC3309 and stars to NGC3311. On the left, the dashed line indicates the linear fit to the NGC3311 points and the dotted–dashed line the fit to those of NGC3309; on the right, the dashed line refers to the global linear fit.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse