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The multiphase circumgalactic medium and its relation to galaxies: an observational perspective

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arxiv 2409.00174 v1 pith:LX3BINVO submitted 2024-08-30 astro-ph.GA

classification astro-ph.GA
keywords galaxiesmediumcircumgalacticessentialevolutiongalaxyhaloionization
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The circumgalactic medium (CGM) is a vital element in galaxies, as it mediates the baryon cycle essential for regulating galaxy activity. It is also highly complex due to the intricate distributions of temperature, density, metallicity, and ionization that make the CGM a multiphase medium. Therefore, learning about the CGM requires combining various observational techniques. This contribution starts by reviewing how absorption spectroscopy, together with modeling of the ionization conditions, yields critical insights into the underlying physical properties of the CGM. Next, the rapidly growing application of imaging and integral field spectroscopy for studying the halo gas in emission, using hydrogen and metal lines as tracers, is examined. Finally, the essential role of the CGM in galaxy evolution is highlighted by considering current studies that directly link galaxies to their halo gas. The novel dimension of how the environment affects the CGM and alters the evolution of galaxies is also investigated.

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Cited by 6 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. GLOW II: A Census of Oxygen in Low-Mass Galaxies

    astro-ph.GA 2026-08 conditional novelty 6.0 of 10

    Low-mass galaxies retain only about 11 percent of the oxygen their stars produced, mostly in gas, and simulations overpredict retention.

  2. Testing the AGN unified model with simulated emission lines from the circumgalactic medium (CGM)

    astro-ph.GA 2025-07 conditional novelty 6.0 of 10

    Using FIRE, CLOUDY, and RASCAS, the authors predict that obscured AGN nebulae are less symmetric, flatter in surface brightness, and broader in Lyα line width at R≥10 kpc than unobscured ones, and that stacking at lea...

  3. The Cosmic Evolution and Spatial Distribution of Multiphase Gas associated with QSOs

    astro-ph.GA 2025-05 conditional novelty 5.0 of 10

    Gas around DESI quasars shows metal absorption that declines with redshift and radius, with an FeII/MgII ratio that grows toward low redshift, indicating progressive metal enrichment.

  4. The Cosmic Evolution of CIV Absorbers at $1.4<z<4.5$: Insights from $100,000$ Systems in DESI Quasars

    astro-ph.CO 2025-04 conditional novelty 5.0 of 10

    A DESI DR2 catalog of 101,487 CIV absorbers shows the absorber path density rising 2 to 5 fold and the CIV mass density rising 3.8 fold from z about 4.5 to z about 1.4.

  5. The Circumgalactic Medium

    astro-ph.GA 2024-12 unverdicted novelty 1.0 of 10

    A comprehensive review of the circumgalactic medium, its multiphase structure, absorption and emission probes, and role in the baryon cycle, containing no new research results.

  6. The Multi-Scale Multi-Phase Circumgalactic Medium: Observed and Simulated

    astro-ph.GA 2024-11 unverdicted novelty 1.0 of 10

    A review chapter and lecture notes summarizing the observational and simulated view of the multiphase circumgalactic medium and the cosmic baryon cycle, with IllustrisTNG-based exercises.

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