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

Published online by Cambridge University Press:  04 August 2017

Elly M. Berkhuijsen  and
Ulrich Klein
Elly M. Berkhuijsen
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, FRG
Ulrich Klein
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, FRG

Extract

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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.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 431 - 434
Copyright
Copyright © Reidel 1985 

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