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• W2852102103 abstract "A technique for studying the star motions inside the open star clusters is proposed. It allows for revealing the details of the spatial and kinematic cluster structure on the basis of precise measurements of the astrometric parameters of the stars. By successively scanning a lot of clusters and applying a uniform technique, a processing pipeline is built. Analysis of such mass processing results reveals the patterns and relationships of the internal arrangement of clusters with their parameters and position in the Galaxy. Actually, the problem has become more interesting by the recently launched space telescope Gaia, in particular, for the membership of star clusters." @default.
• W2852102103 created "2018-07-19" @default.
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• W2852102103 date "2018-01-01" @default.
• W2852102103 modified "2023-09-23" @default.
• W2852102103 title "Aggregation of Knowledge on Star Cluster Structure and Kinematics in Data Intensive Astronomy" @default.
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• W2852102103 doi "https://doi.org/10.1007/978-3-319-96553-6_9" @default.
• W2852102103 hasPublicationYear "2018" @default.
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