Population and dynamical state of the η Chamaeleontis sparse young open cluster

Keyphrases

• Population State 100%
• Open Clusters 100%
• Initial Mass Function 100%
• Dynamical State 100%
• Stellar Masses 50%
• Photometric Surveys 50%
• Main Sequence Stars 50%
• Low-mass 50%
• Dynamical Interaction 50%
• Triple System 50%
• Stellar Clusters 50%
• Mass Segregation 50%
• Young Clusters 50%
• Low-mass Stars 50%
• Interaction Process 50%
• High multiplicity 50%
• T Tauri Stars 50%
• Field Stars 50%
• Pre-main Sequence 50%
• Continuing Studies 50%

Physics

• Open Cluster 100%
• Initial Mass Function 100%
• Stellar Mass 50%
• Main Sequence Stars 50%
• Low-Mass Star 50%
• Young Star Clusters 50%
• T Tauri Stars 50%