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The Motions in the Central Region of NGC 4736∗

Published online by Cambridge University Press:  07 February 2017

P. C. Van Der Kruit
P. C. Van Der Kruit*
Affiliation:
Hale Observatories, Carnegie Institution of Washington, California Institute of Technology, Pasadena, Calif., U.S.A.

Abstract

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Spectroscopic observations of the central part of NGC 4736 show strong noncircular motions connected with the triple radio source. It is also found that a central ring of H II regions is probably expanding at about 30 km s−1.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 58: The Formation and Dynamics of Galaxies , 1974 , pp. 431 - 437
Copyright
Copyright © Reidel 1974 

References

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