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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
fields
astro-ph.SR 2years
2026 2representative citing papers
MWC 656 hosts a hot stripped star companion of 1.48 solar masses instead of a black hole.
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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Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
MWC 656 hosts a hot stripped star companion of 1.48 solar masses instead of a black hole.