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Matteo Cantiello added Figure_3_shows_that_the__.tex
over 8 years ago
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...
Figure 3 shows that the incidence of magnetic suppression increases with
mass, with red giants above 1.6\msol\ showing a remarkable suppression rate
of 50-60\%. These have evolved from main-sequence A-type stars, among which
only up to $\approx 10$\% are observed to have strong fields at their
surfaces \citep{2008CoSka..38..443P}. (see Methods for details:
DISUCSSION OF WHY NOT 100\% AND OR LINKS TO ROTATION AS REFEREE ALLUDES
TO...COULD ALSO BE REFERED TO AFTER 2nd LAST PARA)
We conclude that these magnetic A stars represent only the tip of the
iceberg, and that a much larger fraction of A stars have strong magnetic
fields hidden in their cores.
