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Mapping the asymmetric disc of the Milky Way

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it

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astro-ph.GA 3

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2026 3

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UNVERDICTED 3

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representative citing papers

A correlation predicting galaxies without dark matter

astro-ph.GA · 2026-05-11 · unverdicted · novelty 6.0

Baryonic fraction in certain galaxies correlates with baryonic acceleration as approximately a_bar inverse, placing known dark-matter-deficient galaxies at the high-acceleration extreme and predicting low dark matter content for ultra-diffuse galaxies brighter than 25 mag arcsec^{-2}.

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Showing 3 of 3 citing papers after filters.

  • Rogue Ones: Orbital census of Galactic Cepheids and their Anomalies astro-ph.GA · 2026-06-09 · unverdicted · none · ref 43

    A 6D kinematic census identifies 18 anomalous Cepheids with extreme orbits, including one possibly scattered by globular cluster E3, and finds consistency between dynamical and stellar ages.

  • A correlation predicting galaxies without dark matter astro-ph.GA · 2026-05-11 · unverdicted · none · ref 134

    Baryonic fraction in certain galaxies correlates with baryonic acceleration as approximately a_bar inverse, placing known dark-matter-deficient galaxies at the high-acceleration extreme and predicting low dark matter content for ultra-diffuse galaxies brighter than 25 mag arcsec^{-2}.

  • Tracing the kinematic perturbations of the Milky Way spiral arms with APOGEE DR17 and Gaia DR3 astro-ph.GA · 2026-05-11 · unverdicted · none · ref 52

    Revised radial-velocity response model including V_R,sin and V_R,cos applied to Milky Way kinematic data constrains spiral pitch angle to ~10°, density contrast 5-18%, and pattern speed 10-20 km/s/kpc.