Magnetic field measurements and wind-line variability of OB-type stars

Context. The first magnetic fields in O- and B-type stars that do not belong to the Bp-star class, have been discovered. The cyclic UV wind-line variability, which has been observed in a significant fraction of early-type stars, is likely to be related to such magnetic fields. Aims. We attempt to im...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2008-06, Vol.483 (3), p.857-867
Hauptverfasser:	Schnerr, R. S., Henrichs, H. F., Neiner, C., Verdugo, E., de Jong, J., Geers, V. C., Wiersema, K., van Dalen, B., Tijani, A., Plaggenborg, B., Rygl, K. L. J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics Earth, ocean, space Exact sciences and technology line: profiles Physics stars: activity stars: early-type stars: magnetic fields
Online-Zugang:	Volltext
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