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Tiny-Scale Atomic Structure and the Cold Neutral Medium--Review and Recap

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arxiv astro-ph/0701625 v1 pith:A5QUGOX2 submitted 2007-01-22 astro-ph

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keywords articleatomiccolddiscreteequilibriumneutralpressurestructure
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Almost a decade ago I wrote an article with the same title as this. It focused on the physical properties of the Tiny-Scale Atomic Structure (TSAS) as discrete structures of the Cold Neutral Medium (CNM). To be observable, tiny discrete structures that don't grossly violate pressure equilibrium need two attributes: low temperatures and geometrical anisotropy. Here I update that article. I discuss thermal and pressure equilibrium, ionization, optical lines, H_2 abundance, and evaporation.

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  1. Exploring the Galactic plasma with pulsars in the SKA Era

    astro-ph.HE 2026-07 accept novelty 2.5 of 10

    Pulsars map Galactic, solar-wind, and ionospheric plasma via DM, RM, scintillation, and scattering; SKA-Low/Mid AA4 will push DM precision to ~10^{-8} pc cm^{-3} and transform IISM models.

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