3D SPH simulations show that localized, mildly super-Keplerian equatorial mass ejections with high viscosity reproduce the photometric, spectroscopic, and polarimetric signatures of Be star flicker events.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Population synthesis with detailed reverberation modeling predicts an order of magnitude more detectable middle-aged PWNe for CTAO than currently observed in the TeV band.
citing papers explorer
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The birth of Be star disks III. SPH models of localised mass ejections
3D SPH simulations show that localized, mildly super-Keplerian equatorial mass ejections with high viscosity reproduce the photometric, spectroscopic, and polarimetric signatures of Be star flicker events.
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Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments
Population synthesis with detailed reverberation modeling predicts an order of magnitude more detectable middle-aged PWNe for CTAO than currently observed in the TeV band.