On magnetoacoustic-gravity-inertial (MAGI) waves – II. Application to magnetic and rotating stars
Version of Record online: 15 NOV 2010
© 2010 The Author. Journal compilation © 2010 RAS
Monthly Notices of the Royal Astronomical Society
Volume 410, Issue 2, pages 735–761, January 2011
How to Cite
Campos, L. M. B. C. (2011), On magnetoacoustic-gravity-inertial (MAGI) waves – II. Application to magnetic and rotating stars. Monthly Notices of the Royal Astronomical Society, 410: 735–761. doi: 10.1111/j.1365-2966.2010.17552.x
- Issue online: 30 DEC 2010
- Version of Record online: 15 NOV 2010
- Accepted 2010 August 17. Received 2010 July 16; in original form 2009 August 5
Table 2. Minimum and maximum magnetic fields (Gauss) of non-degenerate stars.
Table 4. Minimum and magnetic field (Gauss) and rotation period (days) of Ap stars.
Table 5. Observed and calculated data for strong non-rotating magnetic stars.
Table 6. Observed and calculated data for fast rotating magnetic stars.
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