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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2 Pith papers cite this work. Polarity classification is still indexing.
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Reports a close stellar encounter rate of 10.6 ± 4.5 per Myr per star within 1 pc for stars in the solar neighborhood, with the GJ 710 approach being rarer than average at one per ~50 Myr.
citing papers explorer
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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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Stellar encounters in the solar neighbourhood and the special case of GJ~710
Reports a close stellar encounter rate of 10.6 ± 4.5 per Myr per star within 1 pc for stars in the solar neighborhood, with the GJ 710 approach being rarer than average at one per ~50 Myr.