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Electron Densities and Nitrogen Abundances in Ionized Gas Derived Using [N ii] Fine-structure and Hydrogen Recombination Lines

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The Central 300 pc of the Galaxy Probed by Infrared Spectra of ${{\rm{H}}}_{3}^{+}$ and CO. I. Predominance of Warm and Diffuse Gas and High H2 Ionization Rate

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HERSCHELGALACTIC PLANE SURVEY OF [N ii] FINE STRUCTURE EMISSION

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Internal structure of spiral arms traced with [C II]: Unraveling the warm ionized medium, H I, and molecular emission lanes

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Kinematics and properties of the central molecular zone as probed with [C ii]

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Evolution of Supernova Remnants Near the Galactic Center

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