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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2026 2representative citing papers
Survey continuation yields FRB20110220A, RRAT J0404+53, new data on J2028+28, and evidence that single-pulse detection rates vary with Galactic coordinates, implying a faint Galactic population.
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The Northern High Time Resolution Universe pulsar survey: III. Single-pulse search continuation, follow-up observations, and initial results
Survey continuation yields FRB20110220A, RRAT J0404+53, new data on J2028+28, and evidence that single-pulse detection rates vary with Galactic coordinates, implying a faint Galactic population.