Difference between revisions of "User:Tohline/Apps/WoodwardTohlineHachisu94"
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[https://youtu.be/t0iqCmbjsNk [[File:Model_O22.png|200px|Click for YouTube Video]] ] | |||
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[https://youtu.be/6s3DMd7yXiA [[File:Model_O22.png|200px|Click for YouTube Video]] ] | |||
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<td align="center">[https://youtu.be/TKkOhdTQrww Table 5, Model O22]</td> | <td align="center">[https://youtu.be/TKkOhdTQrww Table 5, Model O22]</td> | ||
<td align="center">[https://youtu.be/t0iqCmbjsNk Table 5, Model E17]</td> | <td align="center">[https://youtu.be/t0iqCmbjsNk Table 5, Model E17]</td> | ||
<td align="center"> | <td align="center">[https://youtu.be/6s3DMd7yXiA Table 5, Model E29]</td> | ||
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</table> | </table> | ||
Revision as of 18:10, 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.
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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 E17 | Table 5, Model E29 |
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© 2014 - 2021 by Joel E. Tohline |