http://202.127.29.3/~shen/wiki/index.php?action=history&feed=atom&title=STARBIRDS 2026-04-17T01:31:42Z 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=STARBIRDS&diff=3211&oldid=prev 2019-10-16T02:13:08Z

<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;">2019年10月16日 (三) 02:13的版本</td> </tr><tr> <td colspan="2" class="diff-lineno">第4行：</td> <td colspan="2" class="diff-lineno">第4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>*Preliminary ionized gas kinematics are available from an on-going IFU spectroscopic observing campaign (L. van Zee et al. in preparation). </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>*Preliminary ionized gas kinematics are available from an on-going IFU spectroscopic observing campaign (L. van Zee et al. in preparation). </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>*Three galaxies have Chandra X-ray imaging of the hot phase winds (McQuinn et al. 2018)</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>*Three galaxies have Chandra X-ray imaging of the hot phase winds (McQuinn et al. 2018)</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>*KPNO Ha images</div></td> </tr> <!-- diff cache key wikidb2:diff:wikidiff2:1.12:old-3210:rev-3211:1.14.1 --> </table>

Shen http://202.127.29.3/~shen/wiki/index.php?title=STARBIRDS&diff=3210&oldid=prev 2019-10-16T02:11:41Z

<p>创建页面，内容为“*Eleven galaxies are from the STARBurst IRRegular Dwarf Sur- vey (STARBIRDS McQuinn et al. 2015b) *All galaxies have previously derived star formation histories from…”</p> <p><b>新页面</b></p><div>*Eleven galaxies are from the STARBurst IRRegular Dwarf Sur- vey (STARBIRDS McQuinn et al. 2015b)<br /> *All galaxies have previously derived star formation histories from HST observations of their resolved stellar populations (McQuinn et al. 2009, 2010a, 2015b) and measurements of the spatial distribution of recent star formation (McQuinn et al. 2012). <br /> *All galaxies have existing Hi observations to compare with the ionized gas distributions<br /> *Preliminary ionized gas kinematics are available from an on-going IFU spectroscopic observing campaign (L. van Zee et al. in preparation). <br /> *Three galaxies have Chandra X-ray imaging of the hot phase winds (McQuinn et al. 2018)</div>

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