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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0067-0057 umentation, had led to many advances in both CV and LMXB research. The conference provided a forum to review observations from ASCA, EUVE, ROSAT, Ginga and the 978-94-010-6632-7978-94-009-0325-8Series ISSN 0067-0057 Series E-ISSN 2214-7985

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Conference proceedings 1996r-relations between them. The meeting was held at a time when powerful satellite observatories, and rapid improvements in ground based instrumentation, had led to many advances in both CV and LMXB research. The conference provided a forum to review observations from ASCA, EUVE, ROSAT, Ginga and the

formula

Superhumps in the SU UMa Star AK CNCod P. = 0.065(2) d, using the relationship given by Howell & Hurst (1994). The eruption duration was ≳ 10 d, and its amplitude > 6 mag. An abrupt and short luminosity decrease occured ≈ 12 d after maximum. Eleven outbursts have been observed since 1992 January, being the minimum reported lag between

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critique

Oscilloscope as a Diagnostic Tool, is a problem for which there is no universally applicable solution. Velocity measurements are handicapped because the accretion disc about the primary often dominates the optical spectrum. Therefore spectroscopists resort to measuring line profile symmetry in individual spectra of the accretion dis

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