Accretion to magnetized stars through the Rayleigh–Taylor instability: global 3D simulations
Version of Record online: 19 MAR 2008
© 2008 The Authors. Journal compilation © 2008 RAS
Monthly Notices of the Royal Astronomical Society
Volume 386, Issue 2, pages 673–687, May 2008
How to Cite
Kulkarni, A. K. and Romanova, M. M. (2008), Accretion to magnetized stars through the Rayleigh–Taylor instability: global 3D simulations. Monthly Notices of the Royal Astronomical Society, 386: 673–687. doi: 10.1111/j.1365-2966.2008.13094.x
- Issue online: 3 APR 2008
- Version of Record online: 19 MAR 2008
- Accepted 2008 February 11. Received 2008 February 9; in original form 2007 December 9
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