Spiral galaxy centers exhibit complex cold orbital structures such as central drops or steep inner disks, with nuclear disks typically associated with classical bulges rather than pseudo-bulges.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Simulation comparison finds bulgeless galaxies host more centrally concentrated, disc-aligned satellites with steeper faint-end luminosity functions than bulge-dominated controls, reflecting co-evolution and quieter merger histories.
citing papers explorer
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Tracing the dynamical and structural complexity of spiral galaxy centres
Spiral galaxy centers exhibit complex cold orbital structures such as central drops or steep inner disks, with nuclear disks typically associated with classical bulges rather than pseudo-bulges.
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Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
Simulation comparison finds bulgeless galaxies host more centrally concentrated, disc-aligned satellites with steeper faint-end luminosity functions than bulge-dominated controls, reflecting co-evolution and quieter merger histories.