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.