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Similarities and Differences between Magnetic and Non-Magnetic CP Stars

Published online by Cambridge University Press:  12 April 2016

Thierry Lanz
Thierry Lanz*
Affiliation:
NASA Goddard Space Flight Center, Code 681, Greenbelt, MD 20771, USA
*
* NRC-NASA Research Associate

Abstract

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This brief review discusses the similarities between CP stars, focusing on magnetic fields and chemical abundances. New evidence for the presence of a magnetic field with a complex structure in some CP1 stars is presented. Small-scale structures on the surface of these stars may be connected with such a field, and the resulting effects on the curve-of-growth have been investigated. Finally, the changes during evolutionary time-scales on surface abundances are advocated as one possible reason of the large observed scatter in the chemical anomalies inside given groups of CP Stars.

Information

Type
I. General Properties of CP Stars
Information
International Astronomical Union Colloquium , Volume 138: Peculiar versus Normal Phenomena in A-Type and Related Stars , 1993 , pp. 60 - 71
Copyright
Copyright © Astronomical Society of the Pacific 1993

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