Schematic overview of the topics addressed in this paper and their structure in the text. We discuss galaxy properties and formation rates of NMB-type FRB sources in Sect. 3. Subsequently, we discuss the expected kicks and offset, DM and RM evolution, and persistent radio sources in Sect. 4. The galaxy in the left panel is a gri composite from the Sloan Digital Sky Survey, adapted from Masters et al. (2019). The middle panel shows a schematic depiction of an NMB surrounded by expanding material, and the right panel shows two configurations of an NMB, i.e. non-accreting (left) and accreting (right).