  We have identified a new vibrational HCN maser at 89.087 GHz in the
asymptotic giant branch (AGB) star IRAS 15082-4808, a maser which is thought to
trace the innermost region of an AGB envelope. The observations of this maser
at three epochs are presented: two positive detections and one null detection.
The line profile has varied between the positive detections, as has the
intensity of the maser. The major component of the maser is found to be offset
by -2.0+/-0.9 km/s with respect to the systemic velocity of the envelope, as
derived from the 88.631 GHz transition of HCN. Similar blueshifts are measured
in the other 9 sources where this maser has been detected. Maser variability
with pulsation phase has been investigated for the first time using the 10
stars now available. Comparisons with AGB model atmospheres constrain the
position of the formation region of the maser to the region between the
pulsation shocks and the onset of dust acceleration, between 2 and 4 stellar
radii.
