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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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
Empirical power-law relationships are derived to cross-calibrate Ca II K line observations across passbands of 0.1-9 Å and resolutions of 1-6 arcsec using Sunrise III data.
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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Quantifying the effect of passband on observations in the Ca II K line
Empirical power-law relationships are derived to cross-calibrate Ca II K line observations across passbands of 0.1-9 Å and resolutions of 1-6 arcsec using Sunrise III data.