A photometric study of chemically peculiar stars with the STEREO satellites - I. Magnetic chemically peculiar stars

About 10 per cent of upper main-sequence stars are characterized by the presence of chemical peculiarities, often found together with a structured magnetic field. The atmospheres of most of those chemically peculiar stars present surface spots, leading to photometric variability caused by rotational...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2012-02, Vol.420 (1), p.757-772
Hauptverfasser:	Wraight, K. T., Fossati, L., Netopil, M., Paunzen, E., Rode-Paunzen, M., Bewsher, D., Norton, A. J., White, Glenn J.
Format:	Artikel
Sprache:	eng
Schlagworte:	catalogues Magnetic fields Phase transitions Stars & galaxies stars: chemically peculiar stars: rotation techniques: photometric
Online-Zugang:	Volltext
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