Difference between revisions of "User:Tohline/Apps/WoodwardTohlineHachisu94"
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<td align="center">[https://youtu.be/pcfmvIptn8c Table 5, Model O13]</td> | <td align="center">[https://youtu.be/pcfmvIptn8c Table 5, Model O13]</td> | ||
<td align="center">[https://youtu.be/ | <td align="center">[https://youtu.be/kif3ClH6YAs Table 5, Model O14]</td> | ||
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Revision as of 03:32, 27 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.
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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 |
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© 2014 - 2021 by Joel E. Tohline |