首页> 外文期刊>The Astrophysical journal >THE SNAPSHOT HUBBLE U-BAND CLUSTER SURVEY (SHUCS). I. SURVEY DESCRIPTION AND FIRST APPLICATION TO THE MIXED STAR CLUSTER POPULATION OF NGC 4041*
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THE SNAPSHOT HUBBLE U-BAND CLUSTER SURVEY (SHUCS). I. SURVEY DESCRIPTION AND FIRST APPLICATION TO THE MIXED STAR CLUSTER POPULATION OF NGC 4041*

机译:快照易用的U频段集群调查(SHUCS)。 I. NGC 4041混合星团人口的调查描述和首次应用*

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We present the Snapshot Hubble U-band Cluster Survey (SHUCS), a project aimed at characterizing the star cluster populations of 10 nearby galaxies (d 23 Mpc, half within ≈12 Mpc) through new F336W (U-band equivalent) imaging from Wide Field Camera 3, and archival BVI-equivalent data with the Hubble Space Telescope. Completing the UBVI baseline reduces the age-extinction degeneracy of optical colors, thus enabling the measurement of reliable ages and masses for the thousands of clusters covered by our survey. The sample consists chiefly of face-on spiral galaxies at low inclination, in various degrees of isolation (isolated, in group, merging), and includes two active galactic nucleus hosts. This first paper outlines the survey itself, the observational datasets, the analysis methods, and presents a proof-of-concept study of the large-scale properties and star cluster population of NGC?4041, a massive SAbc galaxy at a distance of ≈23 Mpc, and part of a small grouping of six giant members. We resolve two structural components with distinct stellar populations, a morphology more akin to merging and interacting systems. We also find strong evidence of a truncated, Schechter-type mass function, and a similarly segmented luminosity function. These results indicate that binning must erase much of the substructure present in the mass and luminosity functions, and might account for the conflicting reports on the intrinsic shape of these functions in the literature. We also note a tidal feature in the outskirts of the galaxy in Galaxy Evolution Explorer UV imaging, and follow it up with a comprehensive multi-wavelength study of NGC?4041 and its parent group. We deduce a minor merger as a likely cause of its segmented structure and the observed pattern of a radially decreasing star formation rate. We propose that combining the study of star cluster populations with broadband metrics is not only advantageous, but often easily achievable thorough archival datasets.
机译:我们介绍了快照哈勃U波段星团调查(SHUCS),该项目旨在通过新的F336W(相当于U波段)成像来表征10个附近星系(d <23 Mpc,一半在≈12Mpc之内)的星团数量。广角相机3,以及哈勃太空望远镜的档案BVI等效数据。填写UBVI基线可以减少光学色的老化消失性,从而可以测量我们调查涵盖的成千上万个星团的可靠年龄和质量。该样本主要由处于低倾斜,不同隔离度(隔离,成组,合并)的面朝上的螺旋星系组成,并包括两个活跃的银河系核宿主。第一篇论文概述了调查本身,观测数据集,分析方法,并提出了关于NGC?4041(距离≈23的巨大SAbc星系)的大规模性质和星团总数的概念验证研究。 Mpc,以及一个由六个巨型成员组成的小组的一部分。我们解析具有不同恒星种群的两个结构成分,这种形态更类似于合并和相互作用的系统。我们还发现截断的Schechter型质量函数和类似的分段光度函数的有力证据。这些结果表明装仓必须消除质量和光度函数中存在的许多子结构,并且可能解释文献中这些函数的固有形状的相互矛盾的报道。我们还注意到了Galaxy Evolution Explorer UV成像中银河郊区的潮汐特征,并对它进行了NGC?4041及其母体小组的全面多波长研究。我们推断出一次小规模合并可能是其分段结构和观察到的星体形成速率呈放射状下降的模式。我们建议将星团总体的研究与宽带度量结合起来不仅有利,而且通常可以轻松实现详尽的档案数据集。

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