Table 9: Rapidly oscillating Ap stars studied for magnetic field pulsations.
Star $T_{\rm eff}$ $\log~g$ $v~\sin i$ $P_{\rm rot}$ $\left< {\cal B}_z\right>_{\rm aver}$ $\sigma_{z,{\rm aver}}$ $P_{\rm puls}$ $\Delta B_{\rm max}$
  [K]   [km s-1] [d] [G] [G] [min] [mmag]
HD 833681 7960 4.0 33.0 2.85 -847 $\pm$ 108 56 11.6 10
HD 1010652 6600 4.2 3.5   -1014 $\pm$ 72 57 12.1 13
HD 1288981 7998 4.2 13.0 4.48 -239 $\pm$ 136 62 6.8 5
HD 1379491 7030 3.9   >75 y? 2146 $\pm$ 55 51 8.3 3
HD 2016011 7620 4.0   >70 y -1072 $\pm$ 173 55 12.4 3
HD 2175223 6808 4.0 3.0   -686 $\pm$ 111 79 13.9 4

1Hubrig et al. (2000); 2Cowley et al. (2000); 3Hubrig et al. (2002).

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