论文标题
从集群到原始群体：环境星系进化的红外视角
From Clusters to Proto-clusters: the Infrared Perspective on Environmental Galaxy Evolution
论文作者
论文摘要
环境是星系进化的主要驱动因素之一。通过多种机制，它可以控制星系从恒星形成变为静止的关键过程，通常称为“淬火”。但是，尽管它的重要性，但我们仍然对环境驱动的淬火如何在最极端的环境中进行：银河系簇及其祖细胞原始群体也没有清晰的看法。红外功能的最新进展不仅在鉴定这些结构的鉴定方面，而且在整个宇宙时间（原始）群集星系中的静止分析，遮盖的恒星形成和分子气中详细分析。在这篇综述中，我们将讨论有关从观测，红外角度来看（原始）簇中星系淬灭星系的现状。我们对环境星系进化的深入理解来自近乎，中和远红外的独特制度的独特可观察力，这是在向高红移的推动下至关重要的，在这些方案中，大量的星系生长以高度灭绝的，红外的勇敢的星系为主。
Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it can control the critical process of transforming galaxies from star forming to quiescent, commonly termed "quenching". Despite its importance, however, we still do not have a clear view of how environmentally-driven quenching proceeds even in the most extreme environments: galaxy clusters and their progenitor proto-clusters. Recent advances in infrared capabilities have enabled transformative progress not only in the identification of these structures but in detailed analyses of quiescence, obscured star formation, and molecular gas in (proto-)cluster galaxies across cosmic time. In this review, we will discuss the current state of the literature regarding the quenching of galaxies in (proto-)clusters from the observational, infrared perspective. Our improved understanding of environmental galaxy evolution comes from unique observables across the distinct regimes of the near-, mid-, and far-infrared, crucial in the push to high redshift where massive galaxy growth is dominated by highly extincted, infrared-bright galaxies.
