The Evolution of Ap Stars

نویسندگان

  • J. Babel
  • D. Erspamer
چکیده

The many peculiarities of Ap stars (not only chemical ones , but also magnetic field and slow rotation) may vary during the main-sequence evolution of these stars. We review here briefly the evidences found in the last thirty years for such evolution , with an emphasis on the more recent research. The position in the HR diagram of low mass Ap stars with a significant surface magnetic field (as measured by us) is reviewed as well .

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تاریخ انتشار 2008