Abstract
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.
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References
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Monnet, G. (1970). Kinematics of M 33, M 51 and the L. M. C.. In: Becker, W., Contopoulos, G. (eds) The Spiral Structure of Our Galaxy. International Astronomical Union / Union Astronomique Internationale, vol 38. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3275-9_13
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DOI: https://doi.org/10.1007/978-94-010-3275-9_13
Publisher Name: Springer, Dordrecht
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