Dark resonances with widths below 30 Hz have been observed in a rubidium ce
ll filled with neon as buffer gas at room temperature. We compare an approx
imate analytic solution of a Lambda system to our data and show that under
our experimental conditions the presence of the buffer gas reduces the powe
r broadening of the dark resonances by two orders of magnitude. We also pre
sent numerical calculations that take into account the thermal motion and v
elocity-changing collisions with the buffer-gas atoms. The resulting dark-r
esonance features exhibit strong Dicke-type narrowing effects and thereby e
xplain the elimination of Doppler shifts and Doppler broadening, leading to
observation of a single ultranarrow dark line.