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Cool Magnetic CP Stars

  • Saul J. Adelman (a1) and Charles R. Cowley (a1)

Abstract

We review progress in research on the cool magnetic CP stars especially during the past four years. Studies of energy distributions and abundances are analyzed to reveal their systematics. Model atmospheres do not yet accurately describe the average energy distributions much less the variability with the rotational periods of these stars.

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Copyright

References

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Cool Magnetic CP Stars

  • Saul J. Adelman (a1) and Charles R. Cowley (a1)

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