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The Motions in the Central Region of NGC 4736∗
Published online by Cambridge University Press: 07 February 2017
Abstract
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