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Article contents
Global Stability Analysis of an SO Galaxy NGC 3115
Published online by Cambridge University Press: 04 August 2017
Extract
The global modal analysis is applied to a family of models which are consistent with recent dynamical data of NGC 3115. A halo component at least as massive as the disk component is required to explain the apparent lack of spiral structures in NGC 3115.
- Type
- II. Spiral Structure
- Information
- Symposium - International Astronomical Union , Volume 100: Internal Kinematics and Dynamics of Galaxies , 1983 , pp. 125 - 126
- Copyright
- Copyright © Reidel 1983