Abstract
[Abridged] We study the angular-momentum profiles of a statistical sample of halos drawn from a high-resolution N-body simulation of the LCDM cosmology. We find that the cumulative mass distribution of specific angular momentum, j, in a halo of mass Mv is well fit by a universal function, M(
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CITATION STYLE
APA
Bullock, J. S., Dekel, A., Kolatt, T. S., Kravtsov, A. V., Klypin, A. A., Porciani, C., & Primack, J. R. (2001). A Universal Angular Momentum Profile for Galactic Halos. The Astrophysical Journal, 555(1), 240–257. https://doi.org/10.1086/321477
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