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
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- May 1998
- DOI:
- 10.1046/j.1365-8711.1998.01346.x
- Bibcode:
- 1998MNRAS.296..463S
- Keywords:
-
- ACCRETION;
- ACCRETION DISCS;
- HYDRODYNAMICS;
- BINARIES: CLOSE;
- STARS: INDIVIDUAL: IP PEG;
- NOVAE;
- CATACLYSMIC VARIABLES