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• W3105494037 abstract "Using visible, radio, microwave, and sub-mm data, we study several lines of sight toward stars generally closer than 1 kpc on a component-by-component basis. We derive the component structure seen in absorption at visible wavelengths from Ca II, Ca I, K I, CH, CH$^{+}!,$ and CN and compare it to emission from H I, CO and its isotopologues, and C$^{+}$ from the GOT C+ survey. The correspondence between components in emission and absorption help create a more unified picture of diffuse atomic and molecular gas in the interstellar medium. We also discuss how these tracers are related to the CO-dark H$_{2}$ gas probed by C$^{+}$ emission and discuss the kinematic connections among the species observed." @default.
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• W3105494037 date "2018-05-14" @default.
• W3105494037 modified "2023-10-16" @default.
• W3105494037 title "The Connection between Different Tracers of the Diffuse Interstellar Medium: Kinematics" @default.
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• W3105494037 doi "https://doi.org/10.3847/1538-4357/aabae7" @default.
• W3105494037 hasPublicationYear "2018" @default.
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