A theoretical model of a magnetized black hole envelope is developed to explain the broad emission lines and X-ray faintness observed in little red dots using co-rotating plasma clumps and limited X-ray sources.
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4 Pith papers cite this work. Polarity classification is still indexing.
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New EIS effective area curves confirm factor-of-two long-wavelength degradation without fine structure and reveal inverse FIP bias with Fe/H at 0.57 of photospheric value at 10 MK, confirmed by Chandrayaan-2 SXM spectra.
Data-driven MURaM simulations of emerging active region 11640 reproduce key EUV features and find volumetric coronal heating proportional to B squared along with ubiquitous MHD waves.
A review summarizing observational properties, dynamics, and heating implications of transition region loops observed primarily with IRIS, distinct from coronal loops.
citing papers explorer
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A Magnetized Black Hole Envelope Model for Little Red Dots
A theoretical model of a magnetized black hole envelope is developed to explain the broad emission lines and X-ray faintness observed in little red dots using co-rotating plasma clumps and limited X-ray sources.
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Modeling Flare Continuum Emission Observed by Hinode/EIS: Instrument Calibration and Element Composition Results
New EIS effective area curves confirm factor-of-two long-wavelength degradation without fine structure and reveal inverse FIP bias with Fe/H at 0.57 of photospheric value at 10 MK, confirmed by Chandrayaan-2 SXM spectra.
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Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code: Coronal Heating and Dynamics in an Emerging Active Region
Data-driven MURaM simulations of emerging active region 11640 reproduce key EUV features and find volumetric coronal heating proportional to B squared along with ubiquitous MHD waves.
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Magnetic loops in the solar transition region
A review summarizing observational properties, dynamics, and heating implications of transition region loops observed primarily with IRIS, distinct from coronal loops.