NOVA V1425 AQUILAE 1995 - THE EARLY APPEARANCE OF ACCRETION PROCESSESIN AN INTERMEDIATE POLAR CANDIDATE

Continuous CCD photometry of Nova Aquilae 1995 has been performed thro ugh the standard B, V, R and I filters during three nights in 1995 and with the I filter during 18 nights in 1996. The power spectrum of the 1996 data reveals three periodicities in the light curve: 0.2558, 0.0 6005 and 0.079 d, with peak-to-peak amplitudes of about 0.012, 0.014 a nd 0.007 mag respectively. The two shorter periods are absent from the power spectrum of the 1995 light curve, while the long one is probabl y already present in the light curve of that year. We propose that V14 25 Aql should be classified as an intermediate polar cataclysmic varia ble. Accordingly, the three periods are interpreted as the orbital per iod of the underlying binary system, the spin period of the magnetic w hite dwarf and the beat period between them. Our results suggest that, no later than 15 months after the outburst of the nova, accretion pro cesses are taking place in this stellar system. Matter is being transf erred from the cool component, most likely through an accretion disc a nd via accretion columns on to the magnetic poles of the hot component .