“1203.1641”的版本间差异
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（以“unusually high black hole-to-bulge mass ratios in NGC4342 and NGC4291，the observed black hole-to-bulge mass ratios are ~6.9% and ~1.9%, respectively.”为内容创建页面） |
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unusually high black hole-to-bulge mass ratios in NGC4342 and NGC4291，the observed black hole-to-bulge mass ratios are ~6.9% and ~1.9%, respectively. |
unusually high black hole-to-bulge mass ratios in NGC4342 and NGC4291，the observed black hole-to-bulge mass ratios are ~6.9% and ~1.9%, respectively. |
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IFU观测表明晕的质量很大，suggesting that dark matter halos may play a major role in regulating the growth of the supermassive black holes. |
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2013年12月19日 (四) 03:16的最新版本
unusually high black hole-to-bulge mass ratios in NGC4342 and NGC4291，the observed black hole-to-bulge mass ratios are ~6.9% and ~1.9%, respectively.
IFU观测表明晕的质量很大，suggesting that dark matter halos may play a major role in regulating the growth of the supermassive black holes.