Circumgalactic Medium Properties and Galaxy Interactions

Summary

The circumgalactic medium (CGM) is the vast reservoir of diffuse gas that envelops galaxies out to their virial radii, linking the interstellar medium to the intergalactic medium. This multiphase environment comprises cool (T ≈ 10^4 K), warm (T ≈ 10^5 K) and hot (T > 10^6 K) components, enriched by metals ejected in galactic outflows and by inflowing streams of pristine intergalactic gas. Interactions between galaxies—through tidal encounters, minor mergers and group environments—reshape the CGM by triggering shock heating, mixing and turbulence, and by displacing gas clouds. Feedback from star formation and active galactic nuclei drives winds that seed the CGM with metals and momentum, while thermal instabilities and precipitation can cause hot gas to cool in situ, forming clumps that may rain back onto the galaxy. Together, these processes regulate galactic growth, star-formation rates and the cosmic baryon cycle, and they hold the key to resolving the “missing baryons” problem on galactic scales.

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Circumgalactic Medium Properties and Galaxy Interactions publication trend

The graph below shows the total number of articles in circumgalactic medium properties and galaxy interactions across all publications each year (not limited to Nature Index journals).

Technical terms

Circumgalactic Medium (CGM): The diffuse, multiphase gas surrounding a galaxy out to its virial radius, acting as an interface between the galaxy and the intergalactic medium.

Cold-mode accretion: Inflow of relatively cool (T ≲ 10^5 K), low-metallicity gas from the intergalactic medium directly onto a galaxy halo without shock heating to the virial temperature.

Thermal instability: A process in which hot, diffuse gas cools and condenses into denser, cooler clumps when cooling times become shorter than dynamical times.

Turbulence: Random, non-thermal gas motions spanning a cascade of spatial scales, contributing to mixing and energy dissipation in the CGM.

Covering fraction: The fraction of sightlines through a halo that intercept gas above a given column-density threshold for a specified ion or phase.

References

  1. The Cosmic Ultraviolet Baryon Survey: Empirical Characterization of Turbulence in the Cool Circumgalactic Medium. The Astrophysical Journal Letters (2023).
  2. The origin of cold gas in the circumgalactic medium. Astronomy & Astrophysics (2024).
  3. Zooming in on the circumgalactic medium with GIBLE: Resolving small-scale gas structure in cosmological simulations. Monthly Notices of the Royal Astronomical Society (2024).

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