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Titlebook: IUTAM Symposium on Nonlinear Analysis of Fracture; Proceedings of the I J. R. Willis Conference proceedings 1997 Springer Science+Business

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B. Cotterell,K. Y. Lam,Z. Chen,A. G. Atkinsnd that WZ Sge was an eclipsing binary with an 81 min 38 s orbital period. Krzeminski and Kraft (1964, hereafter KK) in the first of many comprehensive analyses of the WZ Sge system to appear in the literature stated “a lower limit to certain detection of orbital velocity changes for the double emis
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Jean Lemaitreaccretion disk and absorptions from the secondary star. This has been shown by Horne et al. (1986). Anticipating the composite nature of the spectrum from the the B-V colour of AH Her, which is intrinsically redder then 0..3, I took spectra of the system in four nights in June 1984 at the 1.2-m-tele
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