Hydrodynamical simulations demonstrate that classical bulges enable bar-driven formation of nuclear stellar disks that bifurcate into pressure-supported nuclear star clusters and rotationally-supported nuclear stellar rings after gas depletion.
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Simulations show that combining QUIJOTE-MFI2 with WMAP and Planck reduces synchrotron spectral index uncertainty by a factor of ~10, curvature uncertainty by ~5, and polarization amplitude uncertainty by ~43 in bright regions while cutting 100 GHz residuals by a factor of 6.
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The SMUGGLE-Ring project: Bar and bulge effects on nuclear disk and ring formation
Hydrodynamical simulations demonstrate that classical bulges enable bar-driven formation of nuclear stellar disks that bifurcate into pressure-supported nuclear star clusters and rotationally-supported nuclear stellar rings after gas depletion.
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Forecasting synchrotron spectral parameters with QUIJOTE-MFI2 in combination with Planck and WMAP
Simulations show that combining QUIJOTE-MFI2 with WMAP and Planck reduces synchrotron spectral index uncertainty by a factor of ~10, curvature uncertainty by ~5, and polarization amplitude uncertainty by ~43 in bright regions while cutting 100 GHz residuals by a factor of 6.