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A 400 tg window of a (u, v) cylinder plots (lef...

A 400 tg window of a (u, v) cylinder plots (left) and the autocorrelations (right) from ...

Nicholas S. Conroy et al, The Astrophysical Journal 1005 1

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A frame from a typical GRMHD model (MAD, a* = 0...

A frame from a typical GRMHD model (MAD, a* = 0.5, i = 30∘, Rhigh = 160) convolved with ...

Nicholas S. Conroy et al, The Astrophysical Journal 1005 1

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A 230 GHz snapshot image from a fiducial Sgr A*...

A 230 GHz snapshot image from a fiducial Sgr A* model (MAD, a* = 0.5, i = 30∘, Rhigh = 1...

Nicholas S. Conroy et al, The Astrophysical Journal 1005 1

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Pattern speed for a toy model in the image doma...

Pattern speed for a toy model in the image domain (shown in warm tones, with color denot...

Nicholas S. Conroy et al, The Astrophysical Journal 1005 1

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Constraints on the sign of ﹩\cos \,i﹩ based on ...

Constraints on the sign of ﹩\cos \,i﹩ based on the direction of the (u, v) pattern speed...

Nicholas S. Conroy et al, The Astrophysical Journal 1005 1

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Measured (u, v) pattern speeds as a function of...

Measured (u, v) pattern speeds as a function of baseline length ρ for nearly face-on (i ...

Nicholas S. Conroy et al, The Astrophysical Journal 1005 1

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Measured (u, v) pattern speeds as a function of...

Measured (u, v) pattern speeds as a function of baseline length, shown for all SANE face...

Nicholas S. Conroy et al, The Astrophysical Journal 1005 1

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Measured (u, v) pattern speeds as a function of...

Measured (u, v) pattern speeds as a function of baseline length, shown for all MAD face-...

Nicholas S. Conroy et al, The Astrophysical Journal 1005 1

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Ωp at the critical curve vs. ΩV A at ρ ≈ 8Gλ, f...

Ωp at the critical curve vs. ΩV A at ρ ≈ 8Gλ, for MAD face-on models (i = 10∘, 170∘). Co...

Nicholas S. Conroy et al, The Astrophysical Journal 1005 1

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Ωp in a v5 retrograde model (MAD, a* = −0.5, i ...

Ωp in a v5 retrograde model (MAD, a* = −0.5, i = 30∘, Rhigh = 160) as a function of diff...

Nicholas S. Conroy et al, The Astrophysical Journal 1005 1

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Illustration of the disk structures and the peb...

Illustration of the disk structures and the pebble drift conditions of the two disks, wi...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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The posterior distributions of the slab-model p...

The posterior distributions of the slab-model parameters of H2O, CO2, C2H2, and HCN for ...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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The best-fit models and the continuum-subtracte...

The best-fit models and the continuum-subtracted spectra (black) of the primary Sz 65 an...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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The observed fluxes of the primary Sz 65 (red) ...

The observed fluxes of the primary Sz 65 (red) and the secondary Sz 66 (blue) over 4.9–5...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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(a) The line-subtracted continuum, (b) line int...

(a) The line-subtracted continuum, (b) line intensity, and (c) Doppler velocity of the e...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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(a) The line-subtracted continuum, (b) line int...

(a) The line-subtracted continuum, (b) line intensity, and (c) Doppler velocity of the e...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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[Ne II] lines of Sz 65 and Sz 66. The rest wave...

[Ne II] lines of Sz 65 and Sz 66. The rest wavelength is indicated by the gray line, and...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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[Ar II] lines of Sz 65 and Sz 66; plotting conv...

[Ar II] lines of Sz 65 and Sz 66; plotting conventions follow Figure 11. The molecular m...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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The continuum-subtracted spectra and the model ...

The continuum-subtracted spectra and the model fluxes in 5.5–7 μm scaled by the best-fit...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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Line diagnostic diagrams for Sz 65 and Sz 66, t...

Line diagnostic diagrams for Sz 65 and Sz 66, together with reference disks from A. Banz...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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Line diagnostics diagram showing accretion lumi...

Line diagnostics diagram showing accretion luminosity derived from mid-IR H I lines vs. ...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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Line diagnostic diagrams showing line ratios vs...

Line diagnostic diagrams showing line ratios vs. the dust disk size R90. The three line ...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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Line diagnostic diagram for non-LTE suppression...

Line diagnostic diagram for non-LTE suppression. Triangles and gray arrows indicate uppe...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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The continuum-subtracted spectra of the primary...

The continuum-subtracted spectra of the primary Sz 65 (red), and the secondary Sz 66 (bl...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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The 10 μm silicate feature of the primary Sz 65...

The 10 μm silicate feature of the primary Sz 65 (upper), and the secondary Sz 66 (lower)...

Jinghuai Yao et al, The Astrophysical Journal 1005 1

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