http://202.127.29.3/~shen/wiki/index.php?action=history&feed=atom&title=N%2FO 2026-05-13T05:12:17Z 本wiki上该页面的版本历史 MediaWiki 1.38.1 http://202.127.29.3/~shen/wiki/index.php?title=N/O&diff=4258&oldid=prev 2025-12-04T10:41:29Z

<p></p> <table style="background-color: #fff; color: #202122;" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="zh-Hans-CN"> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">←上一版本</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">2025年12月4日 (四) 10:41的版本</td> </tr><tr> <td colspan="2" class="diff-lineno">第1行：</td> <td colspan="2" class="diff-lineno">第1行：</td> </tr> <tr> <td class="diff-marker"></td> <td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*https://arxiv.org/abs/1911.00581</div></td> <td class="diff-marker"></td> <td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*https://arxiv.org/abs/1911.00581</div></td> </tr> <tr> <td class="diff-marker"></td> <td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*N/O ratio of 0.46 in GS 3073 at redshift z= 5.55：w can be produced by 1000 - 10,000 M⊙ primordial (Pop III) stars. [https://arxiv.org/abs/2502.04435]</div></td> <td class="diff-marker"></td> <td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*N/O ratio of 0.46 in GS 3073 at redshift z= 5.55：w can be produced by 1000 - 10,000 M⊙ primordial (Pop III) stars. [https://arxiv.org/abs/2502.04435]</div></td> </tr> <tr> <td colspan="2" class="diff-empty diff-side-deleted"></td> <td class="diff-marker" data-marker="+"></td> <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>* All nitrogen-enhanced galaxies have moderate to high gas pressure () and high ionization parameter (), indicating a dense and compact environment. We suggest that super star clusters containing Wolf-Rayet stars and massive stars are the most likely contributors to the elevated nitrogen abundance in these galaxies. arXiv:2512.04043</div></td> </tr> <!-- diff cache key wikidb2:diff:wikidiff2:1.12:old-4187:rev-4258:1.14.1 --> </table>

Shen http://202.127.29.3/~shen/wiki/index.php?title=N/O&diff=4187&oldid=prev 2025-02-11T02:38:47Z

<p></p> <table style="background-color: #fff; color: #202122;" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="zh-Hans-CN"> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">←上一版本</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">2025年2月11日 (二) 02:38的版本</td> </tr><tr> <td colspan="2" class="diff-lineno">第1行：</td> <td colspan="2" class="diff-lineno">第1行：</td> </tr> <tr> <td class="diff-marker"></td> <td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*https://arxiv.org/abs/1911.00581</div></td> <td class="diff-marker"></td> <td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*https://arxiv.org/abs/1911.00581</div></td> </tr> <tr> <td colspan="2" class="diff-empty diff-side-deleted"></td> <td class="diff-marker" data-marker="+"></td> <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>*N/O ratio of 0.46 in GS 3073 at redshift z= 5.55：w can be produced by 1000 - 10,000 M⊙ primordial (Pop III) stars. [https://arxiv.org/abs/2502.04435]</div></td> </tr> <!-- diff cache key wikidb2:diff:wikidiff2:1.12:old-3223:rev-4187:1.14.1 --> </table>

Shen http://202.127.29.3/~shen/wiki/index.php?title=N/O&diff=3223&oldid=prev 2019-11-06T07:34:39Z

<p>创建页面，内容为“*https://arxiv.org/abs/1911.00581”</p> <p><b>新页面</b></p><div>*https://arxiv.org/abs/1911.00581</div>

Shen