Contents of: VI/111/./abstract/GCLAYTON_PROP_2.abs

The following document lists the file abstract/GCLAYTON_PROP_2.abs from catalogue VI/111.
A plain copy of the file (without headers/trailers) may be downloaded.

Many H-deficient stars are detected at near-IR wavelengths, but flux
levels in the mid- and far-IR are uncertain or unknown.  The evolution
of these types of objects suggest periods of enhanced mass-loss
followed by quiescent intervals.  ISO observations of selected H-deficient
stars will present a clearer picture of the evolution of these objects.

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