# Does radiative feedback make faint z>6 galaxies look small?

## TL;DR

This study explores how radiative feedback from young star clusters can explain the extremely compact sizes of faint high-redshift galaxies, suggesting that radiation stabilizes gas clumps and suppresses further star formation.

## Contribution

It demonstrates that radiation from initial star clusters can prevent formation of additional clusters, naturally explaining the small observed sizes of faint z>6 galaxies.

## Key findings

- Radiation from star clusters keeps gas warm and ionized, preventing new cluster formation.
- Small sizes of faint high-z galaxies are due to stabilizing effects of radiation.
- High escape fraction of ionizing radiation predicted for these compact sources.

## Abstract

Recent observations of lensed sources have shown that the faintest ($M_{\mathrm{UV}} \approx -15\,\mathrm{mag}$) galaxies observed at z=6-8 appear to be extremely compact. Some of them have inferred sizes of less than 40 pc for stellar masses between $10^6$ and $10^7\,\mathrm{M}_{\odot}$, comparable to individual super star clusters or star cluster complexes at low redshift. High-redshift, low-mass galaxies are expected to show a clumpy, irregular morphology and if star clusters form in each of these well-separated clumps, the observed galaxy size would be much larger than the size of an individual star forming region. As supernova explosions impact the galaxy with a minimum delay time that exceeds the time required to form a massive star cluster, other processes are required to explain the absence of additional massive star forming regions. In this work we investigate whether the radiation of a young massive star cluster can suppress the formation of other detectable clusters within the same galaxy already before supernova feedback can affect the galaxy. We find that in low-mass ($M_{200} \lesssim 10^{10}\,\mathrm{M}_{\odot}$) haloes, the radiation from a compact star forming region with an initial mass of $10^{7}\,\mathrm{M}_{\odot}$ can keep gas clumps with Jeans masses larger than $\approx 10^{7}\,\mathrm{M}_{\odot}$ warm and ionized throughout the galaxy. In this picture, the small intrinsic sizes measured in the faintest $z=6-8$ galaxies are a natural consequence of the strong radiation field that stabilises massive gas clumps. A prediction of this mechanism is that the escape fraction for ionizing radiation is high for the extremely compact, high-z sources.