'Little red dots' (LRDs) are compact, distant sources with red continua, discovered by JWST. Their color has been attributed either to dust reddening in hot accretion disks or to intrinsic cool emission from dense gas envelopes around accreting supermassive black holes. The lack of temperature diagnostics left the question open. In the spectra of two out of four LRDs at z~2, a rest-frame absorption band at ~1.4 µm was detected, matching the molecular water band of cool stars. Atmospheric models reproduce this feature only at temperatures below 3000 K, confirming a contribution from cool, dense gas (20–30% of the continuum). A composite model with temperatures ~2000–4000 K describes both the absorption and the continuum shape from optical to infrared. The molecular absorption reveals that the red colors of at least some LRDs arise from intrinsic emission rather than dust; consequently, bolometric luminosities and black hole masses may be an order of magnitude lower, offering a new method to probe the emitting gas.
A distant red object usually means one thing: we're seeing a dust veil over a scorching disk falling into a black hole. But when the James Webb split its light into shades, a shadow appeared inside — just like steam from boiling water intercepts rays. This reveals the temperature: the glowing gas isn't white-hot, but merely warm, around 2000–4000 °C. Not a flame, but a moist haze.
Previously, it was thought that the light from such "red dots" was born in a violent whirlpool of matter around a black hole. Now it's clear: the source is a dense cloud of water vapor, and its brightness is tens of times more modest. The mass estimates of central black holes dropped sharply: these are not supergiants, but moderate heavyweights.
The twist: under these conditions, water vapor leaves a unique light signature — a cosmic barcode readable across billions of light years. Thus, water, so distant from life as we know it, becomes a tool unveiling the true nature of distant worlds.
🎯 The trace of water in starlight is like a unique barcode from which we determine the temperature and density of the gas.