Figure 7 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Gravitational Instability and Fragmentation in Collapsar Disks Supports the Formation of Subsolar Neutron Stars

Authors: Yi-Xian Chen, Brian D. Metzger

Yi-Xian Chen and Brian D. Metzger 2025 The Astrophysical Journal Letters 991 .

Provider: AAS Journals

Caption: Figure 7.

Snapshot of the (x, y) profiles through the midplane (z = 0) of density, temperature, dimensionless cooling time, electron fraction Y_e, and μ/kT for the fragmenting simulation O8T1e10. Lengths are expressed in units of the vertical scale height H.

Copyright and Terms & Conditions

Additional terms of reuse

Other Images in This Article

Copyright and Terms & Conditions