Galactic disks evolve secularly through transient, self-quenching spiral episodes excited non-resonantly by mild gradients (cavernae), with high-multiplicity spirals dominating in cold disks and lower-multiplicity ones in warmer disks as heating efficiency changes.
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2 Pith papers cite this work. Polarity classification is still indexing.
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The paper proposes a comprehensive phase-space map of the Milky Way disk from existing and planned surveys plus a consortium to turn those data into a reconstruction of the galaxy's evolutionary history.
citing papers explorer
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Nexae in caverna: the secular evolution of disks via collectively excited, transient spiral structure
Galactic disks evolve secularly through transient, self-quenching spiral episodes excited non-resonantly by mild gradients (cavernae), with high-multiplicity spirals dominating in cold disks and lower-multiplicity ones in warmer disks as heating efficiency changes.
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In Pursuit of Galactic Archaeology: Astro2020 Science White Paper
The paper proposes a comprehensive phase-space map of the Milky Way disk from existing and planned surveys plus a consortium to turn those data into a reconstruction of the galaxy's evolutionary history.