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Properties of H II Regions in the Centers of Nearby Galaxies

  • Authors: Luis C. Ho, Alexei V. Filippenko, and Wallace L. W. Sargent

Ho, Filippenko, & Sargent 1997 The Astrophysical Journal 487 579.

  • Provider: AAS Journals

Caption: Fig. 1.

Integrated absolute blue magnitudes (﹩M^{0}_{B_{T}}﹩, corrected for internal extinction; Ho et al. 1997a) of the host galaxies of H II nuclei for (a) all Hubble types (excluding peculiar classifications), (b) types ranging from S0 to Sbc, and (c) types ranging from Sc to I0. The bins are separated by 0.5 mag.

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