Magnetic fields in Be stars reach up to 460 G, much stronger than the under-100 G values reported in earlier studies, based on new spectropolarimetric observations of seven stars.
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Diffractive interstellar scintillation can produce the observed spectral features in CU Vir's coherent radio emission at 400 MHz for a small emitting region of 0.01 solar radii.
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The magnetic fields in Be stars are stronger than previously suggested
Magnetic fields in Be stars reach up to 460 G, much stronger than the under-100 G values reported in earlier studies, based on new spectropolarimetric observations of seven stars.
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The effect of interstellar scattering on coherent radio emission from stars: the case of CU Vir
Diffractive interstellar scintillation can produce the observed spectral features in CU Vir's coherent radio emission at 400 MHz for a small emitting region of 0.01 solar radii.