  The study of eclipsing binaries is our primary source of measured properties
of normal stars, achieved through analysis of light and radial velocity curves
of eclipsing systems. The study of oscillations and pulsations is increasingly
vital for determining the properties of single stars, and investigating the
physical phenomena active in their interiors. Combining the two methods holds
the promise of establishing stringent tests of stellar evolutionary theory, and
of calibrating model-dependent asteroseismology with empirically measured
stellar properties. I review recent advances and outline future work.
