Titlebook: Cataclysmic Variables and Related Objects; Proceedings of the 1 A. Evans,Janet H. Wood Conference proceedings 1996 Kluwer Academic Publishe

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Distances and Absolute Magnitudes of a Sample of Faint Cataclysmic Variables (1990) in order to establish whether these systems are truely at large distances, or are instead a population of intrinsically faint objects lying relatively nearby. The distances were determined using Bailey’s method (1982) and incorporated the recent .. calibrations by Ramseyer (1994).

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The Place of Origin of the Flickering in Z Chaif eclipses take place (assuming any residual source of noise to be constant in time). The rms-scatter curve is then defined as the function . where σ. is the variance due to flickering and . the variance due to residual noise.

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0067-0057 ral meetings in the area of CVs recently (e. g. Eilat, Abano-Padova, Capetown). However as preparations for the Keele meeting progressed we realized that, while there had been a number of IAU meetings devoted to related and to peripheral topics (such as IAU Colloquium 122 on Classical Novae in 1989,

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Enforcement of the ODR Outcomes,erred time-scales rather than at one cycle length, with a possible secular decrease. In the frequency range 90...900 cycle d. the power spectrum obeys a power law with slope γ ranging from 0.8 to 2.6 for different runs.

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TT Ari-94: A Study of 1.6...60 Minute Variabilityerred time-scales rather than at one cycle length, with a possible secular decrease. In the frequency range 90...900 cycle d. the power spectrum obeys a power law with slope γ ranging from 0.8 to 2.6 for different runs.

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