Difference between revisions of "User:Tohline/Apps/WoodwardTohlineHachisu94"
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[http://adsabs.harvard.edu/abs/1994ApJ...420..247W 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. | [http://adsabs.harvard.edu/abs/1994ApJ...420..247W 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. The following pair of tables list key properties of the set of model tori that were examined: Table 5 gives characteristics of the initial models and Table 6 presents results ascertained from the numerical stability analyses. | ||
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Table extracted from [http://adsabs.harvard.edu/abs/1994ApJ...420..247W J. W. Woodward, J. E. Tohline & I. Hachisu (1994)]<p></p> | Table extracted from [http://adsabs.harvard.edu/abs/1994ApJ...420..247W J. W. Woodward, J. E. Tohline & I. Hachisu (1994)]<p></p> | ||
"''The Stability of Thick, Self-gravitating Disks in Protostellar Systems''"<p></p> | "''The Stability of Thick, Self-gravitating Disks in Protostellar Systems''"<p></p> | ||
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[[File:WTH94_Table5.png| | [[File:WTH94_Table5.png|350px|center|Woodward, Tohline & Hachisu (1994, ApJ, 420, 247)]] | ||
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[[File:WTH94_Table6.png|360px|center|Woodward, Tohline & Hachisu (1994, ApJ, 420, 247)]] | |||
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Revision as of 18:59, 28 November 2015
The Stability of Self-Gravitating Polytropic Tori
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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. The following pair of tables list key properties of the set of model tori that were examined: Table 5 gives characteristics of the initial models and Table 6 presents results ascertained from the numerical stability analyses.
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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 | |
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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 | Table 5, Model O14 | Table 5, Model O15 |
| Table 5, Model O16 | Table 5, Model O17 | Table 5, Model O18 |
| Table 5, Model O22 | Table 5, Model E29 | Table 5, Model E17 |
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