  This is an overview of recent research on meteors and the parent bodies from
which they are produced. While many meteor showers result from material ejected
by comets, two out of the three strongest annual showers (the Geminids and the
Quadrantids) are associated with objects whose physical properties are
apparently those of asteroids. In the last decades dynamical and observational
studies have confirmed the existence of a number of Asteroid-Meteoroid
Complexes, comprising streams and several macroscopic, split fragments.
Spectroscopy of meteor showers has been utilized to investigate the
perihelion-dependent thermal alteration while in interplanetary space. In this
chapter, we review characteristics of the complexes, including those of some
minor streams. The scientific interest is to trace the physical and dynamical
properties of the complexes back to the evolutionary pathways to learn about
the variety of production processes of meteoroids to form streams. We also
discuss open questions in the field for the next decade.
