http://202.127.29.3/~shen/wiki/index.php?action=history&feed=atom&title=Disk_instabilityDisk instability - 版本历史2026-05-13T06:36:37Z本wiki上该页面的版本历史MediaWiki 1.38.1http://202.127.29.3/~shen/wiki/index.php?title=Disk_instability&diff=3989&oldid=prev2023年9月13日 (三) 03:14 Shen2023-09-13T03:14:45Z<p></p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">2023年9月13日 (三) 03:14的版本</td>
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<td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>: linear correlations of normalized mean <ins style="font-weight: bold; text-decoration: none;">[[</ins>clump<ins style="font-weight: bold; text-decoration: none;">]]</ins> sizes with both the gas fraction and the velocity dispersion-to-rotation velocity ratio of the host galaxy.</div></td>
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</table>Shenhttp://202.127.29.3/~shen/wiki/index.php?title=Disk_instability&diff=2618&oldid=prevShen：创建页面，内容为“*violent disk instability model [https://arxiv.org/abs/1703.00458] : linear correlations of normalized mean clump sizes with both the gas fraction and the velocity d...”2017-03-03T06:49:21Z<p>创建页面，内容为“*violent disk instability model [https://arxiv.org/abs/1703.00458] : linear correlations of normalized mean clump sizes with both the gas fraction and the velocity d...”</p>
<p><b>新页面</b></p><div>*violent disk instability model [https://arxiv.org/abs/1703.00458]<br />
: linear correlations of normalized mean clump sizes with both the gas fraction and the velocity dispersion-to-rotation velocity ratio of the host galaxy.</div>Shen