A photometric way to the surface magnetic field of AP stars

Details A photometric way to the surface magnetic field of AP stars A photometric way to the surface magnetic field of AP stars

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....82..230n&link_type=abstract

Astronomy and Astrophysics, vol. 82, no. 1-2, Feb. 1980, p. 230-233.

Astronomy and Astrophysics

Astrophysics

20

A Stars, Binary Stars, Stellar Magnetic Fields, Stellar Spectrophotometry, Abundance, Frequency Distribution, Silicon, Stellar Structure

Scientific paper

It is shown that a definite relation exists between photometric
parameters of peculiarity and surface magnetic fields of slowly rotating
Sr Cr Eu stars. The effect of binarity is discussed and it is shown that
the above relation does not hold for the coolest Ap stars.

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