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Erratum: Spiral structure in the accretion disc of the binary IP Pegasi
Abstract:The paper 'Spiral structure in the accretion disc of the binary IP Pegasi' was published in Mon. Not. R. Astron. Soc. 290 , L28–L32 (1997). Figs 1 and 2 of the paper (grey-scale images) did not reproduce well, and are reprinted here (Fig. 1 overleaf). Colour versions of the images are available on the World Wide Web:http://www-star.st-and.ac.uk/ds10/spirals.html
Keywords:accretion  accretion discs  hydrodynamics  binaries: close  stars: individual: IP Peg  novae  cataclysmic variables  
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