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The star-forming regions (SFRs) in the peculiar galaxies NGC 660, NGC 1512,NGC 4395 and NGC 4618 are studied. The relationships between suchcharacteristics of star forming regions as UV, nearand far-IR fluxes, as wellas in the Halpha and HI lines, surface brightness in these ranges, and thescatter of the radial velocities of ionized and neutral hydrogen areconsidered. It is shown that in all the galaxies considered, the IR fluxes fromSFRs are less than in the "normal" galaxies, but for different reasons: in thegalaxies with signs of recent interaction NGC 660 and NGC 1512, this is due tothe low surface brightness of SFRs; in the lopsided galaxies NGC 4395 and NGC4618, the low brightness of SFRs in the infrared range is due to their compactsize. These differences indicate that the star formation process depends notonly on the morphological type of a galaxy, but also on many other factors.

Study of Star-Forming Regions in the Peculiar Galaxies NGC 660, NGC 1512, NGC 4395, and NGC 4618