Extended emission components are clearly found in the IRAS scan data o
f optically visible oxygen-rich AGE stars which show no 10 mu m silica
te band feature in the IRAS LRS spectra but a strong infrared excess i
n the IRAS photometric data. It is most likely that these stars really
have their circumstellar dust envelopes, which are detached from the
central stars, indicating a halting of mass loss for a significant per
iod.