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Properties of luminous spheroids at redshifts from Keck and HST

机译:来自Keck和HST的红移射频的发光球体的性质

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Three new and still on-going surveys that combine the power of spectroscopy oradaptive optics from the Keck Telescopes with HST images are DEEP, AEGIS, and CATS.The advantages of each for the study of distant bulges are accompanied by a few highlights.We find that the vast fraction of luminous distant bulges appear very red, independent of thebulge luminosity, bulge fraction, disk color, and environment. Yet early-type galaxies appearto be relatively young at redshifts, are less numerous then, host many X-ray AGN's withsome that are highly obscured, and have low but increasing dry-dry and dry-wet merger ratesover time.
机译:三个新的和仍在持续的调查,将光谱技术的力量与HST图像的凯克望远镜与HST图像相结合,宙斯盾和猫。每个用于遥远凸起的研究的优势伴随着几个亮点。我们找到了大部分的发光遥远凸起看起来非常红色,独立于绝缘亮度,凸起分数,磁盘颜色和环境。然而,早期的星系在红移时似乎相对年轻,那么较少,宿主许多X射线AGN的大众,非常模糊,并且具有低但不断增加的干燥干燥和干湿的合并率。

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