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Magnetic fields and X ray emission in pre main sequence stars

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Figure 19: f B against Rossby number for a sample of Sun-like stars (crosses), M0-M6Crosses are sun-like stars Saar (Reiners (2012) showing ReinersLower panel et al., 2009a: reproduced from)
Figure 24: Measurements of M dwarf magnetic fields from Stokes I and Stokes V. Top panel: Averagemagnetic field – Open symbols: measurements from Stokes I; Filled symbols: measurements from Stokes V.Center panel: Ratio between Stokes V and Stokes I measureme
Figure 1.5: Reproduced from Donati & Collier Cameron (1997).Early ZDI reconstruction of themagnetic structure of AB Dor.
Figure 1.6: Reproduced from Morin et al. (2010). Stellar mass against rotation period for the sampleof M dwarfs with published ZDI magnetograms
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