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View Full Version : Magnetic Fields on O-Class Stars



Fraser
2010-Dec-19, 07:50 PM
The primary method by which astronomers can measure magnetic field strength on stars is the Zeeman effect. This effect is the splitting of spectral lines into two due to the magnetic field’s effect on the quantum structure of the orbitals. For massive O-class stars, their spectra are largely featureless in the visual portion of the [...]

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