Radio observations of candidate magnetic O stars

Context.Some O stars are suspected to have to have (weak) magnetic fields because of the observed cyclical variability in their UV wind-lines. However, direct detections of these magnetic fields using optical spectropolarimetry have proven to be very difficult. Aims.Non-thermal radio emission in the...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2007-08, Vol.470 (3), p.1105-1109
Hauptverfasser:	Schnerr, R. S., Rygl, K. L. J., van der Horst, A. J., Oosterloo, T. A., Miller-Jones, J. C. A., Henrichs, H. F., Spoelstra, T. A. Th, Foley, A. R.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology radiation mechanisms: non-thermal radio continuum: stars stars: early-type stars: general stars: magnetic fields stars: mass-loss
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!