Detection of a time-variable relativistic UV outflow at velocities up to 0.3c in quasar J2318, with estimated mass-loss rate and kinetic luminosity above typical feedback thresholds.
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11 Pith papers cite this work. Polarity classification is still indexing.
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Dynamo-generated magnetic fields confine the tachocline against radiative spreading in global simulations, with stronger stable stratification producing longer cycles, deeper penetration via skin effect, and better confinement plus interior spin-down transmission.
A 4.5σ excess RM dispersion of 4.13 ± 0.91 rad m^{-2} is found in 191 Mg II sightlines versus controls, implying model-dependent CGM magnetic fields of 0.4-0.8 μG at projected radii 20-150 kpc and z~1.14.
Dynamo simulations show non-dipolar magnetic field strengths are comparable across dipolar and non-dipolar regimes when scaled by driving power, while the dipole component is an order of magnitude weaker in the non-dipolar regime.
Chaotic Cold Accretion reproduces the observed near-linear black hole mass-bolometric luminosity scaling (slope 0.91) in z>2 quasars while Bondi accretion underpredicts by ~2 dex.
Simulations of evolving galaxies show strong L_nu-SFR and L_nu-V_rot correlations up to z~3, with turbulent magnetic fields dominating at low redshift and large-scale fields growing in importance at higher redshift.
Over 63% of solar active region flux in Cycle 24 clusters in three bands whose drift rates match phase speeds of slow magneto-Rossby waves with toroidal field ~4 kG.
Langevin AIS for multimodal targets has time complexity quadratic in the inverse temperature.
SKA-Mid is predicted to yield samples of 10-100 low-metallicity Lyman continuum emitting galaxies per square degree, enabling multi-wavelength studies of feedback processes linked to ionizing photon escape.
Simulations predict ngVLA at 100 GHz can detect galaxies above 10^9 solar masses at any redshift while SKA low frequencies reach massive dusty galaxies to z=5-7.
Review chapter summarizing the importance of small-scale galactic magnetic fields and proposing SKA observation strategies.
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A New Scaling Law for Non-Dipolar Magnetic Fields in Rapidly Rotating Stars and Planets
Dynamo simulations show non-dipolar magnetic field strengths are comparable across dipolar and non-dipolar regimes when scaled by driving power, while the dipole component is an order of magnitude weaker in the non-dipolar regime.