VLBI astrometry, radial velocities, and adaptive optics data yield an eccentric 2.19-year orbit and total dynamical mass 0.459±0.007 M⊙ for the M-dwarf binary 2MASS J05082729-2101444.
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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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Orbital motion and dynamical mass of the complex periodic variable binary system 2MASS J05082729-2101444
VLBI astrometry, radial velocities, and adaptive optics data yield an eccentric 2.19-year orbit and total dynamical mass 0.459±0.007 M⊙ for the M-dwarf binary 2MASS J05082729-2101444.
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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.