Characterization of the Low-Mass Members in the Praesepe Star Cluster

碩士 === 國立中央大學 === 物理研究所 === 100 === Membership identi cation is the critical rst step to determine the properties of a star cluster. Low-mass members in particular could be used to trace the dynamical history | mass segregation, stellar evaporation, tidal stripping of a star cluster in its Galactic...

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Bibliographic Details
Main Authors: Ping-fang Wang, 王品方
Other Authors: Wen-ping Chen
Format: Others
Language:en_US
Published: 2012
Online Access:http://ndltd.ncl.edu.tw/handle/87560855977182321784