Multiple Generation Star Formation in Cepheus Flare

We present an analysis of the young stellar moving group ASCC 127 using Gaia DR3 data, significantly expanding its membership to 3971 stars—double the number identified in previous studies. Using kinematic and distance criteria, ASCC 127 is divided into five subgroups (Groups 1−5) with ages spanning...

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Bibliographic Details
Main Authors: Fan Wang, Min Fang, Xiaoting Fu, Yang Su, Xuepeng Chen, Shiyu Zhang, Penghui Liu, Xiao-Long Wang, Haijun Tian, Wenyuan Cui, Zhongmu Li
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
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Online Access:https://doi.org/10.3847/1538-3881/add69a
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