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Kinematics of M 33, M 51 and the L. M. C.

Published online by Cambridge University Press:  14 August 2015

G. Monnet*
Affiliation:
Observatoire de Marseille, Marseille, France

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First interferometric results on M 33 in the Hα line at a dispersion of 20 Å/mm, involving 1048 radial velocities, have already been published (Carranza et al., 1968). A new analysis with 3000 measures more will be published soon.

Type
Part I/Spiral Structure in Galaxies
Copyright
Copyright © Reidel 1970 

References

Brandt, J. C.: 1965, Monthly Notices Roy. Astron. Soc. 129, 309.CrossRefGoogle Scholar
Carranza, G., Grillon, R., and Monnet, G.: 1969, Astron. Astrophys. 1, 479.Google Scholar
Carranza, G., Courtès, G., Georgelin, Y., Monnet, G., and Pourcelot, A.: 1968, Ann. Astrophys. 31, 63.Google Scholar
Feast, M.: 1964, Monthly Notices Roy. Astron. Soc. 127, 195.CrossRefGoogle Scholar
Gordon, J.: 1969, Ph.D. Thesis.Google Scholar
Lin, C. C. and Shu, F. H.: 1964, Astrophys. J. 140, 646.CrossRefGoogle Scholar
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