We present ROSAT All-Sky Survey and ROSAT pointed observations (PSPC and HR
I) of a complete sample of 113 bright soft X-ray AGN selected from the ROSA
T Bright Source Catalog. We compare these observations in order to search f
or extreme cases of flux and spectral X-ray variability - X-ray transient A
GN. Three definite transients and one transient candidate are found. The ot
her sources show amplitude variations typically by factors of 2-3 on timesc
ales of years. We found that the variability strength on timescales of days
is a function of the steepness of the X-ray spectrum: steeper X-ray object
s show stronger variability than flat X-ray spectrum sources. We also prese
nt new HRI measurements of our extreme X-ray transients IC 3599 and WPVS007
. We discuss possible models to explain the X-ray transience and the variab
ilities observed in the non-transient sources.