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(a) Face-on gas surface-density map at t = 180 ...

(a) Face-on gas surface-density map at t = 180 Myr with the orbit of the representative ...

Kotaro Kobayashi et al, The Astrophysical Journal Letters 1002 2

(a) Surface-density maps at t = 200 Myr for the...

(a) Surface-density maps at t = 200 Myr for the pseudo-2D (left) and isothermal-3D (righ...

Kotaro Kobayashi et al, The Astrophysical Journal Letters 1002 2

(a) Heat maps of the orbital distribution in th...

(a) Heat maps of the orbital distribution in the Lz–z plane for CND gas (left) and ring ...

Kotaro Kobayashi et al, The Astrophysical Journal Letters 1002 2

(a) Histograms of Lz (left) and ∣z∣ (right) whe...

(a) Histograms of Lz (left) and ∣z∣ (right) when CND and ring particles last crossed R =...

Kotaro Kobayashi et al, The Astrophysical Journal Letters 1002 2

(a) Time evolution of the CND mass (r < 50 pc) ...

(a) Time evolution of the CND mass (r < 50 pc) in the fiducial calculation that includes...

Kotaro Kobayashi et al, The Astrophysical Journal Letters 1002 2

The gravitational densities (ρ = ∇2Φ/4πG) and t...

The gravitational densities (ρ = ∇2Φ/4πG) and their residuals (versus the true densities...

Taavet Kalda and Gregory M. Green, The Astrophysical Journal Letters 1002 2

Performance of the conditional Deep Potential m...

Performance of the conditional Deep Potential method on the dust-free Plummer sphere. To...

Taavet Kalda and Gregory M. Green, The Astrophysical Journal Letters 1002 2

Recovery of the selection function and true spa...

Recovery of the selection function and true spatial density of tracers by the “selection...

Taavet Kalda and Gregory M. Green, The Astrophysical Journal Letters 1002 2

Two-dimensional slices (the z = 0 plane) throug...

Two-dimensional slices (the z = 0 plane) through the three-dimensional dust extinction d...

Taavet Kalda and Gregory M. Green, The Astrophysical Journal Letters 1002 2

Top panel: residuals between our normalizing fl...

Top panel: residuals between our normalizing flow model of the distribution of observed ...

Taavet Kalda and Gregory M. Green, The Astrophysical Journal Letters 1002 2

Sky plots of the “selection function” method’s ...

Sky plots of the “selection function” method’s prediction of the selection function S(x)...

Taavet Kalda and Gregory M. Green, The Astrophysical Journal Letters 1002 2

Left: three-color composite image of Spitzer 8....

Left: three-color composite image of Spitzer 8.0 μm (red), 4.5 μm (green), and 3.6 μm (b...

Chengzhi Meng et al, The Astrophysical Journal 1002 2

Spatial distribution of compact cores/fragments...

Spatial distribution of compact cores/fragments in I19368. The background is ALMA 1.3 mm...

Chengzhi Meng et al, The Astrophysical Journal 1002 2

ALMA 1.3 mm continuum map of I19368. The dashed...

ALMA 1.3 mm continuum map of I19368. The dashed gray contours delineate the boundaries o...

Chengzhi Meng et al, The Astrophysical Journal 1002 2

Maps derived from the VLA NH3 observations over...

Maps derived from the VLA NH3 observations overlaid with the contours of ALMA 1.3 mm con...

Chengzhi Meng et al, The Astrophysical Journal 1002 2

Velocity gradients ∇VLSR,∣∣ as a function of th...

Velocity gradients ∇VLSR,∣∣ as a function of the filamentary structure length Lf. The bl...

Chengzhi Meng et al, The Astrophysical Journal 1002 2

Extracted fragments overlaid on ALMA 1.3 mm con...

Extracted fragments overlaid on ALMA 1.3 mm continuum image. The outlines of the norther...

Chengzhi Meng et al, The Astrophysical Journal 1002 2

Observed molecular line spectra of the clumpy c...

Observed molecular line spectra of the clumpy cloud in I19368. The histogram shows the H...

Chengzhi Meng et al, The Astrophysical Journal 1002 2

Velocity channel maps of the H2CO 3(0, 3)−2(0, ...

Velocity channel maps of the H2CO 3(0, 3)−2(0, 2) line emission above 3 rms (rms ∼ 1.53 ...

Chengzhi Meng et al, The Astrophysical Journal 1002 2

Results of identified filamentary skeletons for...

Results of identified filamentary skeletons for the I19368 region. The background shows ...

Chengzhi Meng et al, The Astrophysical Journal 1002 2

Stellar and tidal evolution for a 3 M⊙ + 3 M⊙ b...

Stellar and tidal evolution for a 3 M⊙ + 3 M⊙ binary with Porb,ZAMS = 5000 days and eZAM...

Veome Kapil et al, The Astrophysical Journal 1002 2

Time evolution of e and Porb for 3 M⊙ + 3 M⊙ bi...

Time evolution of e and Porb for 3 M⊙ + 3 M⊙ binaries over a grid of initial orbital per...

Veome Kapil et al, The Astrophysical Journal 1002 2

Stellar and tidal evolution for a 2.5 M⊙ + 2.5 ...

Stellar and tidal evolution for a 2.5 M⊙ + 2.5 M⊙ binary with Porb,ZAMS = 3 days and eZA...

Veome Kapil et al, The Astrophysical Journal 1002 2

Strength of equilibrium tidal dissipation in ou...

Strength of equilibrium tidal dissipation in our models as a function of the tidal frequ...

Veome Kapil et al, The Astrophysical Journal 1002 2

Tidal dissipation through various channels for ...

Tidal dissipation through various channels for a Sun + hot Jupiter binary system. The da...

Veome Kapil et al, The Astrophysical Journal 1002 2

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