In this study, we give the results of the H spectra obtained from ten different ionized hydrogen sources (Sh2-108, Sh2-119, Sh2-136, Sh2-206, Sh2-228, IC5146, IC444, NGC6572, NGC6960, and NGC7380) in our galaxy using DEFPOS spectrometer. The H spectra provide detailed information about some physical conditions (such as the intensities, the LSR velocities, and the line widths) of the ionized gas in interstellar medium. From these spectra, velocities with respect to the LSR and intensities of the sources were found to be 28.

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