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2013年12月19日 (四) 02:05 Shen
2013-12-19T02:05:45Z
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<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>HST WFC3/IR imaging of 28 Dust Obscured Galaxies (DOGs)</div></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: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;"> </del>We find that only a small fraction (4%, at most11-25%) of the quasar host galaxies are major mergers. </div></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>We find that only a small fraction (4%, at most11-25%) of the quasar host galaxies are major mergers. </div></td>
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<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>Finally, we suggest that the co-incidence of mergers and AGNactivity is luminosity dependent, with only the most luminous quasars beingtriggered mostly by major mergers.</div></td>
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<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>Finally, we suggest that the co-incidence of mergers and AGNactivity is luminosity dependent, with only the most luminous quasars beingtriggered mostly by major mergers.</div></td>
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Shen
http://202.127.29.3/~shen/wiki/index.php?title=1206.4063&diff=827&oldid=prev
Shen：以“Heavily Obscured Quasar Host Galaxies at z~2 are Disks, Not Major Mergers HST WFC3/IR imaging of 28 Dust Obscured Galaxies (DOGs) We find that only a small fract...”为内容创建页面
2013-12-19T02:05:33Z
<p>以“Heavily Obscured Quasar Host Galaxies at z~2 are Disks, Not Major Mergers HST WFC3/IR imaging of 28 Dust Obscured Galaxies (DOGs) We find that only a small fract...”为内容创建页面</p>
<p><b>新页面</b></p><div>Heavily Obscured Quasar Host Galaxies at z~2 are Disks, Not Major Mergers<br />
<br />
HST WFC3/IR imaging of 28 Dust Obscured Galaxies (DOGs)<br />
We find that only a small fraction (4%, at most11-25%) of the quasar host galaxies are major mergers. <br />
<br />
Finally, we suggest that the co-incidence of mergers and AGNactivity is luminosity dependent, with only the most luminous quasars beingtriggered mostly by major mergers.</div>
Shen