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From left to right: meridional slices of the fi...

From left to right: meridional slices of the fiducial (ξTS = 1) model of the composition...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Upper panel: time evolution of the toroidal (so...

Upper panel: time evolution of the toroidal (solid) and poloidal (dashed) components of ...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Evolution of gravitational mass, Mg, and AM for...

Evolution of gravitational mass, Mg, and AM for the remnant core, disk, and total core–d...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Radial profiles of AM transport for the fiducia...

Radial profiles of AM transport for the fiducial model (ξTS = 1) at z = 0. From top to b...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Same as Figure 3, but showing all cases with di...

Same as Figure 3, but showing all cases with different dynamo saturation parameters for ...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Characteristic properties of outflows from the ...

Characteristic properties of outflows from the neutron-star remnant for the fiducial ξTS...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Electron-fraction profiles at ...

Electron-fraction profiles at ﹩\bar{t}=385\,{\rm{ms}}﹩ for the ξTS = 0 (left) and ξTS = ...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Shear viscosity for the TS dynamo at two differ...

Shear viscosity for the TS dynamo at two different postmerger times, ﹩\bar{t}﹩. Shown ar...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Normalized ejected mass distributions for all d...

Normalized ejected mass distributions for all dynamo saturation parameters. From left to...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Mass-ejection rate, ﹩{\dot{M}}_{{\rm{ej}}}﹩, co...

Mass-ejection rate, ﹩{\dot{M}}_{{\rm{ej}}}﹩, computed at a spherical radius of 550 km fo...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Same as Figure 2, but comparing different value...

Same as Figure 2, but comparing different values of χTS.

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Same as Figure 3, but comparing different value...

Same as Figure 3, but comparing different values of χTS.

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Same as Figure 2, but comparing H. C. Spruit (2...

Same as Figure 2, but comparing H. C. Spruit (2002)’s model (blue lines) and J. Fuller e...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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Same as Figure 3, but comparing effects of AM t...

Same as Figure 3, but comparing effects of AM transport at different time moments betwee...

Harry Ho-Yin Ng and Elias R. Most, The Astrophysical Journal Letters 1010 2

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The VDA apparent path length (a) and solar inje...

The VDA apparent path length (a) and solar injection time relative to the simulation inj...

T. Laitinen and S. Dalla, The Astrophysical Journal Letters 1010 2

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The contour shows the simulated proton intensit...

The contour shows the simulated proton intensities as a function of inverse of velocity ...

T. Laitinen and S. Dalla, The Astrophysical Journal Letters 1010 2

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Intensity time profiles for the simulated SEP e...

Intensity time profiles for the simulated SEP event at Δϕ = 0∘ (curves) for the moderate...

T. Laitinen and S. Dalla, The Astrophysical Journal Letters 1010 2

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The VDA apparent path length (a) and solar inje...

The VDA apparent path length (a) and solar injection time (b) of SEPs as a function of t...

T. Laitinen and S. Dalla, The Astrophysical Journal Letters 1010 2

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Our simulated slices of density ((a), (b)) and ...

Our simulated slices of density ((a), (b)) and temperature ((c), (d)) reveal that the wi...

Raphaël Mignon-Risse et al, The Astrophysical Journal Letters 1010 2

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The time evolution (a) and histogram (b) of the...

The time evolution (a) and histogram (b) of the magnetospheric radius, Rm, show bimodali...

Raphaël Mignon-Risse et al, The Astrophysical Journal Letters 1010 2

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Composite SEDs of our models, dominated by the ...

Composite SEDs of our models, dominated by the GRMHD contribution in X-rays, show qualit...

Raphaël Mignon-Risse et al, The Astrophysical Journal Letters 1010 2

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Our simulations naturally exhibit an anticorrel...

Our simulations naturally exhibit an anticorrelation between the jet and X-ray emission....

Raphaël Mignon-Risse et al, The Astrophysical Journal Letters 1010 2

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Simulated X-ray luminosity, LX, increases monot...

Simulated X-ray luminosity, LX, increases monotonically with increasing magnetospheric r...

Raphaël Mignon-Risse et al, The Astrophysical Journal Letters 1010 2

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Spectral energy distributions from the sim-d36 ...

Spectral energy distributions from the sim-d36 model we compare with the high mode (a) a...

Raphaël Mignon-Risse et al, The Astrophysical Journal Letters 1010 2

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Pulsar wind–disk collision leads to enhanced pu...

Pulsar wind–disk collision leads to enhanced pulsar wind power dissipation, as seen thro...

Raphaël Mignon-Risse et al, The Astrophysical Journal Letters 1010 2

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