SKA-VLBI is projected to deliver an order-of-magnitude gain in astrometric precision, enabling detection of thousands of exoplanets around ultra-cool dwarfs, M dwarfs and young stars plus dynamical masses when companions are also imaged.
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2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
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2026 2verdicts
UNVERDICTED 2representative citing papers
Reviews coherent and incoherent radio emission in ordered stellar magnetospheres, links massive-star CBO mechanism to UCD luminosity trends, and predicts SKA detection of ~1000 UCDs to test the hypothesis.
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Ultra-Precise Astrometric Search for Exoplanets with SKA-VLBI
SKA-VLBI is projected to deliver an order-of-magnitude gain in astrometric precision, enabling detection of thousands of exoplanets around ultra-cool dwarfs, M dwarfs and young stars plus dynamical masses when companions are also imaged.