Societies & Publications
An application of the k-th nearest neighbor method to open cluster membership determination
Open clusters are collections of stars that form and evolve together as a group. As open clusters age, their motions through a galaxy can make them difficult to identify compared with background stars. This article introduces a new method which can better differentiate stars that are members of an open cluster compared to background stars, leading to improvements in this field.
http://www.raa-journal.org/raa/index.php/raa/article/view/3073
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Address: 20A Datun Road, Chaoyang District, Beijing, China code: 100012
Tel: 010-64888708 E-mail: naoc@nao.cas.cn