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Radial distributions of constituents in M33, the Galaxy, and M51

  • Elly M. Berkhuijsen (a1) and Ulrich Klein (a1)

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The radial distributions of the surface brightness or column density of thermal and nonthermal radio emission, far-infrared (FIR) emission, blue light, HI and CO in the Sc galaxies M33 and M51 are compared with the corresponding distributions in the Galaxy. Information on the variation of the absorption at Hα and on the variation of the abundance ratio O/H is also shown.

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References

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Radial distributions of constituents in M33, the Galaxy, and M51

  • Elly M. Berkhuijsen (a1) and Ulrich Klein (a1)

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