阻尼Lyman-Alpha星系中金属和恒星的演化

V. Kulkarni
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引用次数: 0

摘要

研究遥远年轻星系的一个独特工具是研究它们在背景类星体光谱中产生的吸收谱线。阻尼Lyman- alpha (DLA)类星体吸收线系统使我们能够经验地追踪星系演化。我们讨论了dla丰度调查的结果及其对星系中全球金属丰度演化的影响。我们还描述了用哈勃太空望远镜(HST)和地面设施进行的深度成像研究,旨在研究吸收器的光度和恒星形成速率。这些观测结果有助于澄清吸收体与星系之间的联系,并阐明在过去80%的宇宙历史中正常星系中恒星和金属的演化。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Evolution of Metals and Stars in Damped Lyman-Alpha Galaxies
A unique tool to investigate distant young galaxies is to study the ab- sorption lines they produce in the spectra of background quasars. The damped Lyman- alpha (DLA) quasar absorption line systems allow us to empirically trace galaxy evo- lution. We discuss results of abundance surveys of DLAs and their implications for the evolution of the global metallicity in galaxies. We also describe deep imaging stud- ies with the Hubble Space Telescope (HST) and ground-based facilities, directed at investigating the luminosities and star formation rates of the absorbers. These obser- vations are helping to clarify the absorber-galaxy connection, and shedding light on the evolution of stars and metals in normal galaxies over the past 80% of th'e cosmic history.
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