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...
Main Authors: | , |
---|---|
Other Authors: | |
Format: | Others |
Language: | en_US |
Published: |
2012
|
Online Access: | http://ndltd.ncl.edu.tw/handle/87560855977182321784 |