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Bayesian Inference of Kinematics and Memberships of Open Cluster

Published online by Cambridge University Press:  17 July 2015

Z.Y. Shao ,
L. Chen ,
J. Zhong  and
J.L. Hou
Z.Y. Shao*
Affiliation:
Shanghai Astronomical Observatory CAS, China
L. Chen
Affiliation:
Shanghai Astronomical Observatory CAS, China
J. Zhong
Affiliation:
Shanghai Astronomical Observatory CAS, China
J.L. Hou
Affiliation:
Shanghai Astronomical Observatory CAS, China
*
e-mail: zyshao@shao.ac.cn
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Abstract

Based on the Bayesian Inference (BI) method, the Multiple-modelling approach is improved to combine coordinative positions, proper motions (PM) and radial velocities (RV), to separate the motion of the open cluster from field stars, as well as to describe the intrinsic kinematic status of the cluster.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 68: The Milky Way Unravelled by Gaia: GREAT Science from the Gaia Data Releases , 2014 , pp. 399
Copyright
© EAS, EDP Sciences, 2015

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