  The G9.5 giant eps Oph shows evidence of radial p-mode pulsations in both
radial velocity and luminosity. We re-examine the observed frequencies in the
photometry and radial velocities and find a best model fit to 18 of the 21 most
significant photometric frequencies. The observed frequencies are matched to
both radial and nonradial modes in the best model fit. The small scatter of the
frequencies about the model predicted frequencies indicate that the average
lifetimes of the modes could be as long as 10-20d. The best fit model itself,
constrained only by the observed frequencies, lies within 1 sigma of eps Oph's
position in the HR-diagram and the interferometrically determined radius.
