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On a possible corrugation of the galactic plane

Published online by Cambridge University Press:  14 August 2015

C. M. Varsavsky  and
R. J. Quiroga
C. M. Varsavsky
Affiliation:
Instituto Argentino de Radioastronomía, Buenos Aires, Argentine
R. J. Quiroga
Affiliation:
Instituto Argentino de Radioastronomía, Buenos Aires, Argentine

Abstract

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We have studied the rotation curve of the Galaxy at different heights below and above the equator. In the course of this work we noticed that the maximum brightness temperature of hydrogen oscillates around the galactic plane following a fairly sinusoidal pattern. It is further noticed that the maximum temperature of hydrogen occurs right on the plane in the regions where the rotation curve has a form indicating solid body rotation. A rotation curve based on points of maximum hydrogen temperature does not differ appreciably from a rotation curve measured on the galactic plane.

Type
Part II/Observations of Spiral Structure in Our Galaxy
Information
Symposium - International Astronomical Union , Volume 38: The Spiral Structure of our Galaxy , 1970 , pp. 147 - 150
Copyright
Copyright © Reidel 1970 

References

Bajaja, E., Garzoli, S., Strauss, F., and Varsavsky, C. M.: 1967, IAU Symposium No. 31, p. 181.CrossRefGoogle Scholar
Shane, N. W. and Bieger-Smith, G. P.: 1966, Bull. Astron. Inst. Netherl. 18, 263.Google Scholar