  A possible sound origin for the photospheric oscillations in the X--ray
bursting sources 1608-522 and 2127+119 is suggested. It is shown that standing
sound waves in an expanding spherical envelope can have periods very close to
the observed ones. The quite large ratio, $\sim$ 10, of the periods in the two
sources is explained in terms of different wave regimes. The relevance of sound
oscillations to the observed QPO in type II bursts of the Rapid Burster is also
discussed.
