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.
M., Tomida, K., White, C
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
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SFUMATO# implements GPU-accelerated AMR for self-gravitational radiation hydrodynamics with new linearized implicit solvers for non-equilibrium chemistry and thermal evolution including dust.
Simulations demonstrate that timescale-based decoupling predictions overestimate separations by a factor of ~3, velocity-based criteria are more accurate, and low-viscosity disks produce decreasing accretion that may identify LISA hosts.
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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SFUMATO#: A GPU-accelerated code for self-gravitational radiation hydrodynamics simulation with adaptive mesh refinement
SFUMATO# implements GPU-accelerated AMR for self-gravitational radiation hydrodynamics with new linearized implicit solvers for non-equilibrium chemistry and thermal evolution including dust.
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The Decoupling of Binaries from Their Circumbinary Disks
Simulations demonstrate that timescale-based decoupling predictions overestimate separations by a factor of ~3, velocity-based criteria are more accurate, and low-viscosity disks produce decreasing accretion that may identify LISA hosts.