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The Distribution of Mass-to-Light Ratio With Radius in M31 and M33

Published online by Cambridge University Press:  14 August 2015

J. E. Baldwin
J. E. Baldwin*
Affiliation:
Cavendish Laboratory, Cambridge, England

Abstract

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New H I observations indicate that the mass-to-light ratios in the disks of M31 and M33 are independent of radius.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 58: The Formation and Dynamics of Galaxies , 1974 , pp. 139 - 140
Copyright
Copyright © Reidel 1974 

References

Emerson, D. T. and Baldwin, J. E.: 1973, Monthly Notices Roy. Astron. Soc. 165, 9P.Google Scholar
Freeman, K. C.: 1970, Astrophys. J. 160, 811.Google Scholar
Warner, P. J., Wright, M. C. H., and Baldwin, J. E.: 1973, Monthly Notices Roy. Astron. Soc. 163, 163.Google Scholar