Figure 4 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

Inferring Globular Cluster Initial Mass Function from Stellar Streams

Authors: Claire S. Ye, Raymond G. Carlberg

Claire S. Ye and Raymond G. Carlberg 2026 The Astrophysical Journal Letters 1007 .

Provider: AAS Journals

Caption: Figure 4.

Similar to Figure 2, but for remnant-cluster-to-initial-mass ratio versus total angular momentum at the present day. The initial clusters start to lose ≳90% mass when their angular momentum L ≲ 1000 kpc km s⁻¹. The vertical dashed line marks 1000 kpc km s⁻¹.

Copyright and Terms & Conditions

Additional terms of reuse

Other Images in This Article

Copyright and Terms & Conditions