arXiv · 2602.01549
Stellar Mass Growth in the First Galaxies: Theory and Observation
Abstract
We compare the growth in stellar mass of galaxies in the $6 2\times10^8 \mathrm{M}_\odot$ in the epoch $8<z<6$ had less than $M_*<\times10^8 \mathrm{M}_\odot$ prior to $z = 8$. Here too we find agreement between models and data, namely that these ~100 Myr 'bursts' had strong in situ growth at $z\le8$, or showed (in Galacticus) substantial stellar and/or gas-rich mergers, and 30-40 Myr 'starbursts' as are common in $z<3$ galaxies. We note that, if a theoretical simulation is unable to pass the test of matching the growth of stellar mass, any success in reproducing the luminosity function is meaningless.
Explore related subjects
Keep this discovery
Alan Dressler, Andrew Benson. 2026-02-02. Stellar Mass Growth in the First Galaxies: Theory and Observation. https://arxiv.org/abs/2602.01549
Cite the original work for its findings. Save a collection to share your selection of sources.