The 2001 Superoutburst of WZ Sagittae: A Clue to the Dynamics of Accretion Disks

Abstract

We examine the light curve of the July-August 2001 superoutburst of WZ Sagittae. During the decline from maximum light the locally defined decay time increases from ~4 d/mag to ~12 d/mag over the first ~15 d of the ~25 d superoutburst, as the system faded from m_V~8.5 to m_V~10. The superoutburst is caused by the sudden accretion of ~10^{24} g of gas onto the white dwarf, and the deviation from exponentiality in the decay light curve is expected qualitatively during a ``viscous decay'' in which the dominant mode of depletion of the gas stored in the accretion disk is accretion onto the central object. In other words, as the mass of the accretion disk decreases, the viscous time scale increases. We show that the data are also quantitatively consistent with the theoretical viscous decay time, both calculated via a simple scaling and also from time dependent calculations, when one adopts standard model parameters for WZ Sge.

13 pages, 2 figures

References in corpus (2)

• The disc instability model for X-ray transients: evidence for truncation and irradiation
• The V-EUV Delay for Dwarf Nova Outbursts: A Case Study for VW Hydri, U Geminorum, and SS Cygni

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