The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing DOI : 10.1111/j.1365-2966.2006.10558.xPeer reviewe
SJ acknowledges support from the German Science Foundation (DFG) Research Unit FOR2544 ‘Blue Planets...
Accepted for publication in MNRAS. A full reproduction package is shared on zenodo in accordance w...
Magnetic fields of cool stars can be directly investigated through the study of the Zeeman effect on...
We report the discovery of a medium-strength (~0.5 kG) magnetic field on the young, massive star ? S...
Accepted for publication in the 'Monthly Notices of the Royal Astronomical Society'We report the dis...
We report the discovery of a medium-strength (similar to 0.5 kG) magnetic field on the young, massiv...
SJ acknowledges support from the German Science Foundation (DFG) Research Unit FOR2544 ‘Blue Planets...
Accepted for publication in MNRAS. A full reproduction package is shared on zenodo in accordance w...
Magnetic fields of cool stars can be directly investigated through the study of the Zeeman effect on...
We report the discovery of a medium-strength (~0.5 kG) magnetic field on the young, massive star ? S...
Accepted for publication in the 'Monthly Notices of the Royal Astronomical Society'We report the dis...
We report the discovery of a medium-strength (similar to 0.5 kG) magnetic field on the young, massiv...
SJ acknowledges support from the German Science Foundation (DFG) Research Unit FOR2544 ‘Blue Planets...
Accepted for publication in MNRAS. A full reproduction package is shared on zenodo in accordance w...
Magnetic fields of cool stars can be directly investigated through the study of the Zeeman effect on...