How Galaxies Exhale Their Gas ✛ ✎

Original: "Outflows in the Early Universe: Neutral gas Absorption in Galaxies at z > 3 from low-resolution JWST Spectroscopy"
arXiv:2607.20606v1 · 2026-07-22 · arXiv non-exclusive · independent analysis · 2 min
The James Webb Space Telescope caught distant galaxies in the act of ejecting cold gas, starving themselves of fuel for new stars.

Just two billion years after the Big Bang, massive galaxies are already exhaling their gas back into space. The JWST detected this by the yellow trace of sodium — a color familiar to everyone from streetlights. This trace appears when cold gas absorbs light. In galaxies, this gas is the primary fuel for birthing new stars.

The yellow sodium lines in a galaxy's spectrum are like a signature of cold interstellar gas (the tenuous medium between stars), hidden behind dense cosmic dust.

To understand where the fuel goes, astronomers led by Matteo Sapori studied 811 distant galaxies with redshifts (stretching of light due to the expansion of the universe) from 3 to 7. They used spectroscopy — a method that splits light into colors, much like a raindrop creates a rainbow. In each spectrum, they searched for a dip at the wavelength of sodium. A confident signal turned up in only 20 galaxies, but these were the most massive and dusty. Among those whose star formation (the process of star birth) had already slowed, the fraction with such an exhalation reached 43%. Estimates show that gas flows out faster than it transforms into new stars — up to 12 solar masses per year.

In galaxies where almost no new stars are born, the neutral wind blows especially often — nearly every other one.

So what pushes the gas out? Most likely, powerful radiation from young massive stars, and sometimes an active galactic nucleus — a supermassive black hole devouring matter at the center. This wind drains the reservoirs of cold fuel, and star formation fizzles out. Thus early galaxies transition from a tumultuous youth to a calm maturity. Two yellow streaks in the rainbow of light tell us how the universe learned to breathe, billions of years before our time.

The yellow sodium lines that betray a galactic exhalation are the very ones that make streetlights glow amber.

N_{\text{NaI}} = 1.13 \times 10^{20} \frac{EW}{f_{lu} \lambda_{lu}^2} \, \text{cm}^{-2}
Relationship between the equivalent width of the Na I D absorption line (EW) and the number of atoms along the line of sight (N_NaI), assuming optically thin gas.
\dot{M}_{\text{out}} = 1.2 \, M_\odot \, \text{yr}^{-1} \left( \frac{\Omega}{0.4 \cdot 4\pi} \right) \left( \frac{R_{\text{out}}}{1 \, \text{kpc}} \right) \left( \frac{v_{\text{out}}}{200 \, \text{km/s}} \right) \left( \frac{EW}{1 \, \text{Å}} \right)
Mass outflow rate (Mdot_out) as a function of the outflow opening solid angle (Omega), radius (R_out), velocity (v_out), and measured equivalent width.
Scientists
Alan GuthAlexander FriedmannAndrei LindeGeorges LemaîtreJames PeeblesAdam Riess
Concepts
early universe galaxies galactic outflow early universe star formation high redshift galaxies dust transparency anomaly ultra fast outflow star formation gas outburst roman jwst red sources starburst dust grain gas accretion james webb space telescope interstellar space dark ages non gaussianity dwarf galaxy void outflow