Pulsation in cool main-sequence Am stars is a rare phenomenon observed in a
few marginal Am stars and only one classical Am star. The chemically pecul
iar star HD 13079 is shown to be pulsating with a 78-min period and a peak-
to-peak B amplitude of 0.02 mag, The Hipparcos parallax, uvby beta photomet
ry and pulsations together suggest that HD 13079 is an Am star near the zer
o-age main sequence, and that it is a fundamental-mode pulsator on the red
edge of the instability strip.