Planet-hosting stars display a bimodal S_phot distribution (peaks at 0.12 and 0.44 rad d^{-1}) absent in controls, with overall enhancement, interpreted as two regimes of magnetic activity coherence.
, year = 1955, month = sep, volume =
2 Pith papers cite this work. Polarity classification is still indexing.
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Review summarizing observational data on the Milky Way's magnetic field structure, including spiral alignment, halo components, turbulence, and correlations with interstellar gas and dust.
citing papers explorer
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Bimodality in Rotational Modulation of Planet-Hosting Stars
Planet-hosting stars display a bimodal S_phot distribution (peaks at 0.12 and 0.44 rad d^{-1}) absent in controls, with overall enhancement, interpreted as two regimes of magnetic activity coherence.
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The magnetic field of the Milky Way: an observational perspective
Review summarizing observational data on the Milky Way's magnetic field structure, including spiral alignment, halo components, turbulence, and correlations with interstellar gas and dust.