How did massive galaxies stop forming stars within 700 Myr?
This text mentions work from 2024 on. Those parts were partly written without a live literature search and have not been checked by an editor yet.
In plain words
JWST found massive galaxies that had already finished forming stars when the universe was under a billion years old. Making that many stars and then stopping so quickly is hard to reproduce in models.
Precise statement
JWST has confirmed massive quiescent galaxies up to $z = 7.29$ (RUBIES-UDS-QG-z7, $M_{*} >\sim 10^{10} M_{\mathrm{sun}}$); quiescent number densities exceed most models by up to $\sim 1\,\mathrm{dex}$ at $z \sim 3-5$, and the abundance implied at $z \sim 7$ is more than 100 times any model prediction (Weibel et al. 2025). Determine whether standard Lambda-CDM halo abundances with physical feedback can produce such galaxies, which requires star formation rates of hundreds of $M_{\mathrm{sun}}/\mathrm{yr}$ followed by quenching within $\sim 10^{8}\,\mathrm{yr}$, or whether stellar masses and ages are biased by the assumed initial mass function or AGN light.
What would settle it
Spectroscopic stellar masses, ages and number densities for a complete sample at $z > 4$ compared with simulations that use the same selection, giving agreement or a quantified excess.
Status in the literature
Unverified note: it names recent work and was partly written without a live literature search; it awaits a check by an editor.
As of 2026 initial mass function variation, AGN contamination of the light and small-sample statistics are proposed explanations; none is established.
Parent problems
- Special case of What stops star formation in massive galaxies? · open · from revision 1
Results
No results have been posted on this problem yet.
Post a result · how results are checked
Sign in to follow or save this problem
Comments (0)
Comments are not records: they are not signed, stamped or logged. How comments work
No comments yet.
Sign in to comment.