All Research

The First RELHIC? Cloud-9 is a Starless Gas Cloud

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Read the paperDOI: 10.3847/2041-8213/ae1584

TL;DR

Imagine the universe is filled with invisible scaffolding made of dark matter - we can't see it directly, but it provides the framework for everything else. Scientists have long predicted that some of these invisible structures should be filled with gas but never light up with stars, like empty lots in a city that have utilities but no buildings. Cloud-9 is the first confirmed example of this phenomenon - it's essentially an "invisible galaxy" made of dark matter and gas, sitting near the spiral galaxy M94. Using powerful telescopes, researchers confirmed it has no stars (making it invisible to normal light) but contains about a million times the mass of our Sun in hydrogen gas. This discovery is important because it proves our theories about how the universe is structured are correct, and helps explain why some cosmic neighborhoods remain dark while others become brilliant galaxies.

Abstract Five-hundred-meter Aperture Spherical Telescope observations have recently identified a compact H i cloud (hereafter Cloud-9) in the vicinity of the spiral galaxy M94. This identification has been confirmed independently by Very Large Array and Green Bank Telescope observations. Cloud-9 has the same recession velocity as M94, and is therefore at a similar distance (∼4.4 Mpc). It is compact ( ∼1′ radius, or ∼1.4 kpc), dynamically cold ( W 50 = 12 km s −1 ), nonrotating, and fairly massive, with an H i mass of ∼10 6 M ⊙ . Here we present deep Hubble Space Telescope/Advanced Camera for Surveys imaging designed to search for a luminous stellar counterpart. We visually rule out the presence of any dwarf galaxy with stellar mass exceeding 10 3.5 M ⊙ . A more robust color–magnitude diagram-based analysis conservatively rules out a 10 4 M ⊙ stellar counterpart with 99.5−8.2+0.5 % confidence. The nondetection of a luminous component reinforces the interpretation that this system is a reionization-limited H i cloud (RELHIC); i.e., a starless dark matter halo filled with hydrostatic gas in thermal equilibrium with the cosmic ultraviolet background. Our results make Cloud-9 the leading RELHIC candidate of any known compact H i cloud. This provides strong support for a cornerstone prediction of the Lambda cold dark matter model, namely the existence of gas-filled starless dark matter halos on subgalactic mass scales, and constrains the present-day threshold halo mass for galaxy formation.

  • 1Cloud-9 is confirmed as the first robust candidate for a reionization-limited H i cloud (RELHIC), a starless dark matter halo filled with neutral hydrogen gas
  • 2Deep Hubble Space Telescope imaging rules out any stellar counterpart with mass exceeding 10^4 solar masses with 99.5% confidence
  • 3The system has properties consistent with theoretical predictions: compact size (~1.4 kpc radius), dynamically cold (W50 = 12 km/s), and massive H i content (~10^6 solar masses)
  • 4Cloud-9 provides strong observational support for the Lambda cold dark matter model's prediction of gas-filled starless dark matter halos on subgalactic scales
  • 5The discovery constrains the present-day threshold halo mass for galaxy formation at approximately 10^9.7 solar masses
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