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Equatorial-plane density map for t ≃ 67 days, f...

Equatorial-plane density map for t ≃ 67 days, for simulation BH 2L. The upper panel show...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Evolution of the three principal spatial dimens...

Evolution of the three principal spatial dimensions of the debris cloud λi with time dur...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Pressure distribution in the equatorial plane (...

Pressure distribution in the equatorial plane (left panel) and in several meridional pla...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Mean density (normalized by ...

Mean density (normalized by ﹩{\rho }_{{\rm{BH}}}={M}_{{\rm{BH}}}{r}_{* }^{-3}﹩) within t...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Multi-exposure plot showing the evolution of th...

Multi-exposure plot showing the evolution of the stellar debris from the initial hydrost...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Three-dimensional rendering of the field lines ...

Three-dimensional rendering of the field lines at t = 2.4 days, i.e., stage S2. Color sh...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Pressure distribution (shown by transparent gra...

Pressure distribution (shown by transparent gray surfaces) and magnetic field lines plot...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Eccentricity distribution in the runs BH 2 and ...

Eccentricity distribution in the runs BH 2 and BH 2L after the formation of the fallback...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Time spans and remapping sequences in the simul...

Time spans and remapping sequences in the simulation. Dotted lines show remappings, and ...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Magnetic field energies in the units of total h...

Magnetic field energies in the units of total heat (integrated over stellar material) as...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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One-sided magnetic field flux as a function of ...

One-sided magnetic field flux as a function of time. Different curves represent differen...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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One-sided toroidal magnetic flux throughout BH ...

One-sided toroidal magnetic flux throughout BH 2 as a function of φ and time. The upper ...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Simulation BHz at t ≃ 485 days. Panels show equ...

Simulation BHz at t ≃ 485 days. Panels show equatorial cross sections of rotation veloci...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Magnetic field correlations over azimuth and ti...

Magnetic field correlations over azimuth and time (t = 480−520 days, 50 frames) normaliz...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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PDSs of the three magnetic field components, Bϖ...

PDSs of the three magnetic field components, Bϖ, Bφ, and Bz, averaged over 50 frames of ...

Pavel Abolmasov et al, The Astrophysical Journal 1001 1

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Gradients of measured quantities of NGC 1266’s ...

Gradients of measured quantities of NGC 1266’s outflow. Top row: from the left to right,...

Sebastian Lopez et al, The Astrophysical Journal 1001 1

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Top left: broadband (0.5–7.0 keV) X-ray image o...

Top left: broadband (0.5–7.0 keV) X-ray image of NGC 1266 overlaid with the regions used...

Sebastian Lopez et al, The Astrophysical Journal 1001 1

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Left: combined spectra from all three observati...

Left: combined spectra from all three observations extracted from the northern regions a...

Sebastian Lopez et al, The Astrophysical Journal 1001 1

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Top: three-color image of NGC 1266, where red i...

Top: three-color image of NGC 1266, where red is the SMA CO(2–1) observations from K. Al...

Sebastian Lopez et al, The Astrophysical Journal 1001 1

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Left: four-color image of NGC 1266. The HST dat...

Left: four-color image of NGC 1266. The HST data show the disk in the F110W (blue), F140...

Sebastian Lopez et al, The Astrophysical Journal 1001 1

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MUSE data products used in this paper, all of w...

MUSE data products used in this paper, all of which were clipped to a signal-to-noise ra...

Sebastian Lopez et al, The Astrophysical Journal 1001 1

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First and second: gradients with distance of th...

First and second: gradients with distance of the median ne and P/k values from the MUSE ...

Sebastian Lopez et al, The Astrophysical Journal 1001 1

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The flat-equivalent circular velocity of extrag...

The flat-equivalent circular velocity of extragalactic systems as a function of stellar ...

Stacy S. McGaugh et al, The Astrophysical Journal 1001 1

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The stellar mass fraction as a function of stel...

The stellar mass fraction as a function of stellar mass (top) and the baryonic mass frac...

Stacy S. McGaugh et al, The Astrophysical Journal 1001 1

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The observed flat velocity Vf as it relates to ...

The observed flat velocity Vf as it relates to the fitted V200 for pseudo-isothermal (le...

Stacy S. McGaugh et al, The Astrophysical Journal 1001 1

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