On the surface distribution of chemical anomalies of AP stars in spectroscopic binary systems

Details On the surface distribution of chemical anomalies of AP stars in spectroscopic binary systems On the surface distribution of chemical anomalies of AP stars in spectroscopic binary systems

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..68..283k&link_type=abstract

Astrophysics and Space Science, vol. 68, no. 2, Apr. 1980, p. 283-294.

Astronomy and Astrophysics

Astrophysics

8

A Stars, Binary Stars, Chemical Composition, Magnetic Stars, Stellar Spectrophotometry, Abundance, Anomalies, Frequency Distribution, Histograms, Periodic Variations

Scientific paper

By estimating the orbital inclinations of non-eclipsing Ap spectroscopic binaries with periods less than 13 days, we can obtain a marked statistical result on the frequency distribution of the inclinations which strongly suggests that the abundance anomalies of Ap components tend to concentrate towards the stellar polar region. This would provide a critical test for models of Ap stars

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