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Galactic Radio Astronomy
Ionization and heating mechanisms are reviewed; some of them apply to the interstellar medium as a whole, others only to localized regions. Cooling processes are briefly summarized. Results are given from a recent model calculation for an intercloud medium heated by X-rays.doi:10.1007/978-94-010-2263-7_9 fatcat:qzu5qzgdprdcxda35lfypzms7e