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AE Aqr
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XY Ari
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de Martino et al 1999

Bibinfo (this paper at ADS)
de Martino, D., Silvotti, R., Buckley, D.A.H., Gaensicke, B.T., Mouchet, M., Mukai, K., Rosen, S.R. 1999, A&A 350, 517-528.
Type
Observational: IUE and HST spectroscopy.
Object(s)
FO Aqr.
Results
Fluxes were modulated more strongly on the orbital than the spin period in 1995 UV (IUE and HST) data; in comparison with 1990, the accretion curtain seems to have shrunk. These are consistent with a disk-overflow mode (from the pure disk mode in 1990).


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