Spectroscopic members of the M92 stream yield a Milky Way bar pattern speed of 29.1 +0.7/-0.4 km s^{-1} kpc^{-1}.
The case of the tidal stream of the Hyades
3 Pith papers cite this work, alongside 17 external citations. Polarity classification is still indexing.
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astro-ph.GA 3years
2026 3representative citing papers
Extensive Gaia, CaHK, UNIONS, SDSS, and DELVE searches find no observational evidence that Boötes III is the progenitor of the Styx stream.
Test-particle simulations show that Galactic bar pattern speed systematically deflects open-cluster tidal tail orientations, with NGC 2632 and Hyades tails disfavouring moderate speeds.
citing papers explorer
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Constraining the Galactic bar using the M92 stellar stream
Spectroscopic members of the M92 stream yield a Milky Way bar pattern speed of 29.1 +0.7/-0.4 km s^{-1} kpc^{-1}.
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Characterizing the disruption of B\"ootes III: a missing link in the Galactic halo?
Extensive Gaia, CaHK, UNIONS, SDSS, and DELVE searches find no observational evidence that Boötes III is the progenitor of the Styx stream.
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Bar-induced deflection of open cluster tidal tails
Test-particle simulations show that Galactic bar pattern speed systematically deflects open-cluster tidal tail orientations, with NGC 2632 and Hyades tails disfavouring moderate speeds.