Erratum: Spiral structure in the accretion disc of the binary IP Pegasi

Details Erratum: Spiral structure in the accretion disc of the binary IP Pegasi Erratum: Spiral structure in the accretion disc of the binary IP Pegasi

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.296..463s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 296, Issue 2, pp. 463-464.

Astronomy and Astrophysics

Astronomy

15

Accretion, Accretion Discs, Hydrodynamics, Binaries: Close, Stars: Individual: Ip Peg, Novae, Cataclysmic Variables

Scientific paper

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

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