用KMOS3D观测星系的早期生长和生命周期

IF 0.3 Q4 COMMUNICATION
N. F. Schreiber, D. Wilman, E. Wisnioski, M. Fossati, J. Mendel, R. Bender, R. Genzel, A. Beifiori, S. Belli, G. Brammer, A. Burkert, J. Chan, R. Davies, R. L. Davies, M. Fabricius, A. Galametz, R. Herrera-Camus, P. Lang, D. Lutz, I. Momcheva, T. Naab, E. Nelson, S. Price, A. Renzini, R. Saglia, S. Seitz, Taro Shimizu, A. Sternberg, L. Tacconi, K. Tadaki, H. Übler, P. Dokkum, S. Wuyts
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引用次数: 1

摘要

近红外光谱仪是研究星系演化的有力工具。我们完成了多年的KMOS 3D观测,
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Witnessing the Early Growth and Life Cycle of Galaxies with KMOS3D
Near-infrared spectrographs are powerful tools for investigating galaxy evolution. We on our completed multi-year KMOS 3D survey of a ,
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Jurnal The Messenger
Jurnal The Messenger COMMUNICATION-
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