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Theory of spots on chemically peculiar stars

EAS Publications Series, 2014
Surface inhomogeneities are found in many stars. In active sun-like stars and cool giants temperature spots similar to that found in the Sun are recovered from the inversion of spectroscopic data. M-dwarfs also show highly inhomogeneous surface structures in polarized light and photometric variability that are believed to be connected with cool regions
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Atmospheric Variations in Chemically Peculiar Stars

1989
The expression ‘Chemically Peculiar Stars’ was established by Preston in 1974 to group together the various types of stars with abnormal chemical composition on the upper main sequence. In this volume Maitzen (1989) gives a compilation of the variety of photometric and spectroscopic properties of all subtypes of CP stars.
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Magnetic field structures in chemically peculiar stars

Astrophysical Bulletin, 2011
We report the results of magnetic field modelling of around 50 CP stars, performed using the “magnetic charges” technique. The modelling shows that the sample reveals four main types of magnetic configurations: 1) a central dipole, 2) a dipole, shifted along the axis, 3) a dipole, shifted across the axis, and 4) complex structures. The vast majority of
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A Plethora of New, Magnetic Chemically Peculiar Stars From LAMOST DR4

Astronomy and Astrophysics, 2020
Ernst Paunzen, Stefan Hummerich
exaly  

Multiplicity Among Chemically Peculiar Stars - II. Cool Magnetic Ap Stars

Astronomy and Astrophysics, 2002
F Carrier, P North, J Bäbel
exaly  

On the Detection of Chemically Peculiar Stars Using a Photometry

Astronomy and Astrophysics, 2005
Ernst Paunzen, H M Maitzen
exaly  

The Kepler View of Magnetic Chemically Peculiar Stars

Astronomy and Astrophysics, 2018
Ilya Yakunin   +2 more
exaly  

Magnetic Field Topology of the Unique Chemically Peculiar Star CU Virginis

Astronomy and Astrophysics, 2014
Coralie Neiner   +2 more
exaly  

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