Time-series interferometry shows the Mira R Car pulsates steadily in the fundamental mode, while the red supergiant VX Sgr experiences episodic shock-driven mass loss and a pulsation-mode change.
A., Laplace, E., Schneider, F
4 Pith papers cite this work. Polarity classification is still indexing.
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Radiative-transfer models of SN2023ixf require a 0.2 solar-mass cold dense shell plus rising dust mass to match its nebular-phase UV-optical-IR evolution to 1000 days.
3D MHD simulations of CCSN remnants from RSG and WR stars show faster shocks from photoionization and CSM expansion, plus coherent reflected shocks in WR cases, with weakly magnetized bubbles limiting PeV acceleration.
Radiative-transfer models of SN2023ixf require prolonged CSM interaction and a cold dense shell to match its multi-wavelength photospheric evolution from 20 to 120 days.
citing papers explorer
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VLTI-GRAVITY measurements of cool evolved stars: II. Pulsation properties and mass-loss process of the Mira star R Car and the red supergiant VX Sgr
Time-series interferometry shows the Mira R Car pulsates steadily in the fundamental mode, while the red supergiant VX Sgr experiences episodic shock-driven mass loss and a pulsation-mode change.
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SN2023ixf: ultraviolet-to-infrared radiative-transfer modeling of the nebular-phase evolution until 1000 days
Radiative-transfer models of SN2023ixf require a 0.2 solar-mass cold dense shell plus rising dust mass to match its nebular-phase UV-optical-IR evolution to 1000 days.
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Multi-Dimensional MHD simulations of young Core-Collapse Supernova Remnants
3D MHD simulations of CCSN remnants from RSG and WR stars show faster shocks from photoionization and CSM expansion, plus coherent reflected shocks in WR cases, with weakly magnetized bubbles limiting PeV acceleration.
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SN2023ixf: Radiative-transfer modeling of the photospheric phase evolution from the ultraviolet to the infrared
Radiative-transfer models of SN2023ixf require prolonged CSM interaction and a cold dense shell to match its multi-wavelength photospheric evolution from 20 to 120 days.