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Top: long-term light curve of ASASSN-14ds. The ...

Top: long-term light curve of ASASSN-14ds. The blue and red dots are ASAS-SN V- and g-ba...

Albert Bruch et al, Research Notes of the AAS 10 7

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An illustration of the geometric setup of our s...

An illustration of the geometric setup of our simulations (a), followed by the detectabi...

Morgan Micharski and Chris Richardson, Research Notes of the AAS 10 7

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Flux density of the continuum emission from PDS...

Flux density of the continuum emission from PDS 70 c obtained from multiwavelength ALMA ...

Yuhito Shibaike et al, The Astrophysical Journal Letters 1006 1

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Comparisons of the predictions by the Drift mod...

Comparisons of the predictions by the Drift model (left panel) and Ring model (right pan...

Yuhito Shibaike et al, The Astrophysical Journal Letters 1006 1

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Radial distribution of the dust properties in t...

Radial distribution of the dust properties in the CPD of PDS 70 c in the Drift and Ring ...

Yuhito Shibaike et al, The Astrophysical Journal Letters 1006 1

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Radial distribution of the midplane temperature...

Radial distribution of the midplane temperature and profiles calculated without the vari...

Yuhito Shibaike et al, The Astrophysical Journal Letters 1006 1

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Same as Figure 3, but with colors representing ...

Same as Figure 3, but with colors representing different quantities. The colors in the l...

Yuhito Shibaike et al, The Astrophysical Journal Letters 1006 1

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Properties of flares— luminosity, temperature, ...

Properties of flares— luminosity, temperature, and duration— as functions of AGN luminos...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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Properties of EM flares in the TQM model with M...

Properties of EM flares in the TQM model with MSMBH = 108 M⊙ and ...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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Same as Figure 8, but for the SG model with ...

Same as Figure 8, but for the SG model with ...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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A comparison of various characteristic sizes in...

A comparison of various characteristic sizes in the TQM model. Solid, dashed, and dotted...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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Similar to Figure 12, but for properties of bre...

Similar to Figure 12, but for properties of breakout emission associated with jets launc...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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Same as Figure 10, but for the SG model.

Same as Figure 10, but for the SG model.

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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Same as Figure 14, but showing the dependence o...

Same as Figure 14, but showing the dependence on mBH, fb, ηj, and p.

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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Same as Figure 8, but showing the dependence on...

Same as Figure 8, but showing the dependence on several parameters. The left to right co...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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The fraction of the radial distance from the SM...

The fraction of the radial distance from the SMBH (logarithmic scale) for cases transiti...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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The trapping radius (dashed curves) versus circ...

The trapping radius (dashed curves) versus circularization radius (solid curves) for acc...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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The mass of a BH at which the ADIOS state is re...

The mass of a BH at which the ADIOS state is realized due to accretion growth prior to k...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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A schematic illustration of EM flares associate...

A schematic illustration of EM flares associated with compact-object mergers within an A...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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Same as Figure 2, but for the SG model.

Same as Figure 2, but for the SG model.

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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Same as Figure 4, but for the SG model, and als...

Same as Figure 4, but for the SG model, and also showing a sub-Eddington AGN (lower pane...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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Same as Figure 6, shown for the SG model on a u...

Same as Figure 6, shown for the SG model on a uniform logarithmic grid with models separ...

Hiromichi Tagawa et al, The Astrophysical Journal 1006 2

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Predicted timescales of stellar bar formation. ...

Predicted timescales of stellar bar formation. Theoretical simulations of bar formation ...

Leindert A. Boogaard et al, The Astrophysical Journal Letters 1006 1

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Spectral energy distribution model of GN20. The...

Spectral energy distribution model of GN20. The best-fit SED model from MAGPHYS with the...

Leindert A. Boogaard et al, The Astrophysical Journal Letters 1006 1

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Stellar bar identification. The ellipticity and...

Stellar bar identification. The ellipticity and PA of the stellar light isophotes at res...

Leindert A. Boogaard et al, The Astrophysical Journal Letters 1006 1

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