Difference between revisions of "User:Tohline/Apps/WoodwardTohlineHachisu94"
| Line 97: | Line 97: | ||
</table> | </table> | ||
=See Also= | |||
<ul> | |||
<li>[[User:Tohline/Apps/ImamuraHadleyCollaboration#Characteristics_of_Unstable_Eigenvectors_in_Self-Gravitating_Tori|Characteristics of Unstable Eigenvectors in Self-Gravitating Tori]]</li> | |||
</ul> | |||
<br /> | <br /> | ||
{{LSU_HBook_footer}} | {{LSU_HBook_footer}} | ||
Revision as of 16:45, 11 March 2020
The Stability of Self-Gravitating Polytropic Tori
|
|---|
| | Tiled Menu | Tables of Content | Banner Video | Tohline Home Page | |
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.
|
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 | |
 |
 |
Online Movies
| Figure 1: Animation Sequences to Supplement Figure 10 of WTH94 (click on security-lock icon or caption model name to go to YouTube) | ||
|---|---|---|
| ||
| Table 5, Model O15 | Table 5, Model O14 | |
| Table 5, Model E17 | Table 5, Model E29 | |
|
Caption to Fig. 10 from WTH94: "<math>~\phi_m - r</math>" diagrams illustrating the azimuthal structure of the four specific eigenmodes that were found to be dynamically unstable in our modeled disks. (a) The m = 1 P-mode, shown here as it developed in model O15 <math>~[M_d/M_c = 1; ~T/|W| = 0.316];</math> (b) The m = 1 A-mode, shown here as it developed in model O14 <math>~[M_d/M_c = 1; ~T/|W| = 0.251];</math> (c) The m = 2 I-mode, shown here as it developed in model E17 <math>~[M_d/M_c = 5; ~T/|W| = 0.256];</math> (d) The m = 2 L-mode, shown here as it developed in model E29 <math>~[M_d/M_c = 0.2; ~T/|W| = 0.447]\, .</math> |
||
| Figure 2: Five Additional Animation Sequences to Supplement Table 5 of WTH94 (click on security-lock icon or caption model name to go to YouTube) | ||||
|---|---|---|---|---|
| Table 5, Model O13 | Table 5, Model O16 | Table 5, Model O17 | Table 5, Model O18 | Table 5, Model O22 |
See Also
|
|
|---|
|
© 2014 - 2021 by Joel E. Tohline |