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Flickering Mapping of the Cataclysmic Variables

Published online by Cambridge University Press:  22 February 2018

A. Bortoletto
Affiliation:
Departamento de Física, Universidade Federal de Santa Catarina, Trindade, 88040-900, Florianópolis, SC, Brazil ([email protected])
R. Baptista
Affiliation:
Departamento de Física, Universidade Federal de Santa Catarina, Trindade, 88040-900, Florianópolis, SC, Brazil ([email protected])

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We report results of simulation to evaluate the ability of the eclipse mapping method to reproduce the spatial distribution of flickering in cataclysmic variables stars.

Flickering is a fast intrinsic brightness scintilation occurring on time scales from seconds to minutes with amplitudes of 0.01 - 1 mag. Flickering is observed in all sources believed to be powered by accretion is considered a fundamental signature of accretion. Nevertheless, it is one of the least undestood aspects of the accretion process.

Type
The Contributed Papers
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Baptista, R, Steiner, J., Cieslinski, D., 1994. ApJ, 433 Google Scholar
Bennie, P.; Hilditch, R.; Horne, K., 1996. In: Cataclysmic Variables and related objects, proc. of IAU Colloquium 158, p33, eds Evans, A. & Wood, J.H., Kluwer Google Scholar
Bruch, A., 1996. In: Cataclysmic Variables and related objects, proc. of IAU Colloquium 158, p35, eds Evans, A. & Wood, J.H., Kluwer Google Scholar
Bruch, A., 2000., MNRAS, 389, 998 Google Scholar
Horne, K., 1985., MNRAS, 213, 129 Google Scholar
Horne, K., Stiening, R. F., 1985., MNRAS, 216, 933 Google Scholar