Radio observations of candidate magnetic O stars

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 th...

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Bibliographic Details
Main Authors: Schnerr, R., Rygl, K., van der Horst, A., Oosterloo, T., Miller-Jones, James, Henrichs, H., Spoelstra, T., Foley, A.
Format: Journal Article
Published: EDP Sciences 2007
Subjects:
radiation mechanisms: non-thermal
stars: general
stars: mass-loss
stars: magnetic fields
radio continuum: stars
stars: early-type
Online Access:http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2007A%2526A...470.1105SFUL
http://hdl.handle.net/20.500.11937/24456

Internet

http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2007A%2526A...470.1105SFUL
http://hdl.handle.net/20.500.11937/24456

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