The nature of the magnetic field of CP stars

Details The nature of the magnetic field of CP stars The nature of the magnetic field of CP stars

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..342d&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Mar.-Apr. 1990, p. 342-350. In Russian.

Astronomy and Astrophysics

Astronomy

4

Peculiar Stars, Stellar Evolution, Stellar Magnetic Fields, Stellar Envelopes, Stellar Mass

Scientific paper

The masses of Cp stars with strong magnetic fields tend to exceed 2 solar masses. An analysis of the early stages of stellar evolution indicates that efficient convection is absent in the envelopes of stars with masses above 2 solar masses. Therefore, only these stars of the main sequence can conserve a strong relict magnetic field. To conserve the strong magnetic field, intense sources of ionization (SN or OB stars) must be present in the vicinity.

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