N-body and SPH simulations show that gas accretion along a galactic warp can generate global, long-lived phase spirals in the stellar disc with amplitudes comparable to those observed by Gaia.
S., Dekel, A., Kolatt, T
3 Pith papers cite this work. Polarity classification is still indexing.
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A new cylindrical cosmological simulation method with radially varying resolution enables self-consistent N-body evolution in S¹×ℝ² topology for systems mismatched to cubic periodicity.
Constrained Local Group hydrodynamical simulations predict up to 8 HI-detectable dark galaxies within 2.5 Mpc of the Milky Way.
citing papers explorer
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Phase spirals induced by the gas warp
N-body and SPH simulations show that gas accretion along a galactic warp can generate global, long-lived phase spirals in the stellar disc with amplitudes comparable to those observed by Gaia.
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Cylindrical cosmological simulations with StePS
A new cylindrical cosmological simulation method with radially varying resolution enables self-consistent N-body evolution in S¹×ℝ² topology for systems mismatched to cubic periodicity.
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HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
Constrained Local Group hydrodynamical simulations predict up to 8 HI-detectable dark galaxies within 2.5 Mpc of the Milky Way.