HVC and IVC gas in the halo of the Milky Way
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🌌 astro-ph
keywords
haloabsorptionabundancesanalysecaiicombineconditionsdistribution
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We combine CaII/NaI absorption and HI 21 cm emission line measurements to analyse the metal abundances, the distribution, the small-scale structure, and the physical conditions of intermediate- and high-velocity gas in the Galactic halo.
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