Spiral instabilities: mode saturation and decay

Author:

Sellwood J A1,Carlberg R G2

Affiliation:

1. Steward Observatory, University of Arizona , 933 N Cherry Ave, Tucson AZ 85722, USA

2. Department of Astronomy and Astrophysics, University of Toronto , ON M5S 3H4, Canada

Abstract

ABSTRACT This paper continues a series reporting different aspects of the behaviour of disc galaxy simulations that support spiral instabilities. The focus in this paper is to demonstrate how linear spiral instabilities saturate and decay, and how the properties of the disc affect the limiting amplitude of the spirals. Once again, we employ idealized models that each possess a single instability that we follow until it has run its course. Remarkably, we find a tight correlation between the growth rate of the mode and its limiting amplitude, albeit from only six simulations. We show that non-linear orbit deflections near corotation cause the mode to saturate, and that the more time available in a slowly growing mode creates the critical deflections at lower amplitude. We also find that scattering at the inner Lindblad resonance is insignificant until after the mode has saturated. Our objective in this series of papers, which we believe we have now achieved, has been to develop a convincing and well-documented account of the physical behaviour of the spiral patterns that have been observed in simulations by others, and by ourselves, for many decades. Understanding the simulations is an important step towards the greater objective, which is to find observational evidence from galaxies that could confront the identified mechanism.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Cross-method Analysis of Corotation Radii Data Set for Spiral Galaxies;Research in Astronomy and Astrophysics;2024-07-01

2. Bottom’s Dream and the Amplification of Filamentary Gas Structures and Stellar Spiral Arms;The Astrophysical Journal;2024-04-29

3. Families of eccentric resonant orbits in galaxy discs: backbones for bars and spirals;Monthly Notices of the Royal Astronomical Society;2024-02-15

4. Saturation of spiral instabilities in disc galaxies;Monthly Notices of the Royal Astronomical Society;2024-01-30

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