Author(s): , , , ,
Institution(s): 1. Shanghai Astronomical Observatory
Based on the Bayesian inference (BI) method, the mixture-modeling approach is improved to combine all kinematic data, including the coordinative position, proper motion (PM) and radial velocity (RV), to separate the motion of the cluster from field stars in its area, as well as to describe the intrinsic kinematic status. Meanwhile, the membership probabilities of individual stars are determined as by product results. This method has been testified by simulation of toy models and it was found that the joint usage of multiple kinematic data can significantly reduce the missing rate of membership determination, say from ~15% for single data type to 1% for using all position, proper motion and radial velocity data.
By combining kinematic data from multiple sources of photometric and redshift surveys, such as WIYN and APOGEE, M67 and NGC188 are revisited. Mass segregation is identified clearly for both of these two old open clusters, either in position or in PM spaces, since the Bayesian evidence (BE) of the model, which includes the segregation parameters, is much larger than that without it. The ongoing work is applying this method to the LAMOST released data which contains a large amount of RVs cover ~200 nearby open clusters. If the coming GAIA data can be used, the accuracy of tangential velocity will be largely improved and the intrinsic kinematics of open clusters can be well investigated, though they are usually less than 1 km/s.