伯克利87/ON2方向的星团形成

IF 27.8 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
D. de la Fuente, C. Rom'an-Z'uniga, E. Jim'enez-Bail'on, J. Alves, Miriam García, Sean Venus
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引用次数: 0

摘要

上下文。解开年轻恒星群的视线排列对于恒星形成复合体的观测研究至关重要。这个任务在天鹅座- x的子区域中尤其困难,因为在这个区域中,位于不同距离的几个组成部分是重叠的:伯克利87年轻的大质量星团,鲜为人知的[DB2001] Cl05嵌入星团,以及ON2恒星形成复合体,它们反过来由几个Hii区域组成。目标提供一种方法,对年轻天体进行详尽的普查,以一致地处理在消光和距离上的巨大差异。方法。OMEGA2000对伯克利87 / ON2场的近红外观测与盖亚、钱德拉、斯皮策和赫舍尔的档案数据以及文献中的交叉鉴定合并在一起。为了解决视距重叠引起的不完全性效应和选择偏差,我们对现有的消光估计和年轻目标分类方法进行了改进,并定义了固有变红指数(Rint),这是一种新的工具,用于将固有红源与由于消光而导致的红外颜色过量的源分开。我们还介绍了一种基于Rint的寻找年轻恒星物体的新方法。结果。我们发现了571个天体,它们的分类与最近或正在形成的恒星有关。连同其他有距离或消光估计的点源,我们编制了一个包含3005个天体的目录,用于进一步的成员工作。伯克利87的新距离为(1673±17)pc,估计为13个具有精确Gaia EDR3视差的光谱成员的中位数。结论。我们方法的灵活性,特别是在Rint定义方面,可以克服由大消光和距离变化引起的光度偏差,以便获得年轻源的均匀目录。将我们的方法应用于伯克利87 / ON2场的多波长普查结果将作为解开重叠种群的基础。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Clustered star formation toward Berkeley 87/ON2
Context. Disentangling line-of-sight alignments of young stellar populations is crucial for observational studies of star-forming complexes. This task is particularly problematic in a Cygnus-X subregion where several components, located at different distances, are overlapped: the Berkeley 87 young massive cluster, the poorly-known [DB2001] Cl05 embedded cluster, and the ON2 star-forming complex, in turn composed of several Hii regions. Aims. To provide a methodology for building an exhaustive census of young objects that can consistently deal with large differences in both extinction and distance. Methods. OMEGA2000 near-infrared observations of the Berkeley 87 / ON2 field are merged with archival data from Gaia, Chandra, Spitzer, and Herschel, as well as cross-identifications from the literature. To address the incompleteness effects and selection biases that arise from the line-of-sight overlap, we adapt existing methods for extinction estimation and young object classification, and we define the intrinsic reddening index, Rint, a new tool to separate intrinsically red sources from those whose infrared color excess is caused by extinction. We also introduce a new method to find young stellar objects based on Rint. Results. We find 571 objects whose classification is related to recent or ongoing star formation. Together with other point sources with individual estimates of distance or extinction, we compile a catalog of 3005 objects to be used for further membership work. A new distance for Berkeley 87, (1673 ± 17) pc, is estimated as a median of 13 spectroscopic members with accurate Gaia EDR3 parallaxes. Conclusions. The flexibility of our approach, especially regarding the Rint definition, allows to overcome photometric biases caused by large extinction and distance variations, in order to obtain homogeneous catalogs of young sources. The multi-wavelength census that results from applying our methods to the Berkeley 87 / ON2 field will serve as a basis for disentangling the overlapped populations.
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来源期刊
The Astronomy and Astrophysics Review
The Astronomy and Astrophysics Review 地学天文-天文与天体物理
CiteScore
45.00
自引率
0.80%
发文量
7
期刊介绍: The Astronomy and Astrophysics Review is a journal that covers all areas of astronomy and astrophysics. It includes subjects related to other fields such as laboratory or particle physics, cosmic ray physics, studies in the solar system, astrobiology, instrumentation, and computational and statistical methods with specific astronomical applications. The frequency of review articles depends on the level of activity in different areas. The journal focuses on publishing review articles that are scientifically rigorous and easily comprehensible. These articles serve as a valuable resource for scientists, students, researchers, and lecturers who want to explore new or unfamiliar fields. The journal is abstracted and indexed in various databases including the Astrophysics Data System (ADS), BFI List, CNKI, CNPIEC, Current Contents/Physical, Chemical and Earth Sciences, Dimensions, EBSCO Academic Search, EI Compendex, Japanese Science and Technology, and more.
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