  We recently reported strong evidence for solar-like oscillations in the G0 IV
star eta Boo (Kjeldsen et al. 1995, AJ 109, 1313). We measured small
temperature fluctuations produced by oscillations through their effect on the
equivalent widths of the Balmer lines. Here we address several issues that were
raised at this conference. In particular, we show a power spectrum made without
applying a high-pass filter to the observations. This spectrum shows increased
noise at low frequencies, as expected, and the oscillation signature is still
clearly visible.
