User:Tohline/Apps/WoodwardTohlineHachisu94

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The Stability of Self-Gravitating Polytropic Tori

Whitworth's (1981) Isothermal Free-Energy Surface
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J. W. Woodward, J. E. Tohline, & I. Hachisu (1994; hereafter WTH94) used nonlinear numerical hydrodynamic techniques to examine the relative stability of self-gravitating, polytropic tori toward the development of nonaxisymmetric structure.


Table extracted from J. W. Woodward, J. E. Tohline & I. Hachisu (1994)

"The Stability of Thick, Self-gravitating Disks in Protostellar Systems"

ApJ, vol. 420, pp. 247-267 © American Astronomical Society

Woodward, Tohline & Hachisu (1994, ApJ, 420, 247)

Online Movies

Figure 1: Animation Sequences to Supplement Table 5 of WTH94

(click on security-lock icon or caption model name to go to YouTube)

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Table 5, Model O13    

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Table 5, Model O16 Table 5, Model O17  


 

Whitworth's (1981) Isothermal Free-Energy Surface

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Recommended citation:   Tohline, Joel E. (2021), The Structure, Stability, & Dynamics of Self-Gravitating Fluids, a (MediaWiki-based) Vistrails.org publication, https://www.vistrails.org/index.php/User:Tohline/citation