arXiv · 2411.17312
A Shallow Slope for the Stellar Mass--Angular Momentum Relation of Star-Forming Galaxies at $1.5 < z < 2.5$
Abstract
We present measurements of the specific angular momentum $j_\star$ of 41 star-forming galaxies at $1.5 1$ in some cases) in low-mass haloes that decrease with increasing mass, suggesting a significant role of efficient angular momentum transport in these gas-rich systems, aided by the removal of low-$j_\star$ gas via feedback-driven outflows in low-mass galaxies.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Juan M. Espejo Salcedo, Karl Glazebrook, Deanne B. Fisher, Sarah M. Sweet, Danail Obreschkow, N. M. Förster Schreiber. 2024-11-26. A Shallow Slope for the Stellar Mass--Angular Momentum Relation of Star-Forming Galaxies at $1.5 < z < 2.5$. https://doi.org/10.1093/mnras%2Fstae2647
Cite the original work for its findings. Save a collection to share your selection of sources.