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Best-fit model to the observed λ = 1.3 mm flux ...

Best-fit model to the observed λ = 1.3 mm flux of Juno. The orange circles with error ba...

Jian-Yang Li et al, The Planetary Science Journal 7 3

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Model lightcurves of Juno with various thermal ...

Model lightcurves of Juno with various thermal inertias as listed in the legend and diff...

Jian-Yang Li et al, The Planetary Science Journal 7 3

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The distributions of all 19 best-fit parameters...

The distributions of all 19 best-fit parameters for Juno that are statistically acceptab...

Jian-Yang Li et al, The Planetary Science Journal 7 3

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Modeled thermal inertia with respect to grain s...

Modeled thermal inertia with respect to grain size for S-type asteroid materials. Panel ...

Jian-Yang Li et al, The Planetary Science Journal 7 3

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Minimum thermal inertia allowed by the B. Gundl...

Minimum thermal inertia allowed by the B. Gundlach & J. Blum (2013) model (solid line) a...

Jian-Yang Li et al, The Planetary Science Journal 7 3

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Modeled thermal inertia with respect to grain s...

Modeled thermal inertia with respect to grain size radius. The different colors reflect ...

Jian-Yang Li et al, The Planetary Science Journal 7 3

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Derived loss tangent for Juno (symbols) compare...

Derived loss tangent for Juno (symbols) compared to the values predicted by models (curv...

Jian-Yang Li et al, The Planetary Science Journal 7 3

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Ratios of the observed flux to the model for Ju...

Ratios of the observed flux to the model for Juno, assuming uniform thermal and dielectr...

Jian-Yang Li et al, The Planetary Science Journal 7 3

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Simulated flux density distribution of Juno at ...

Simulated flux density distribution of Juno at λ = 1.3 mm at three rotational phases. Th...

Jian-Yang Li et al, The Planetary Science Journal 7 3

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Large misalignment of position angles between c...

Large misalignment of position angles between continuous jets and discrete ejecta in GRS...

Wu Jiang et al, The Astrophysical Journal Letters 1000 2

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Top: schematic plots of warped disk and continu...

Top: schematic plots of warped disk and continuous jet or ejecta in GRS 1915+105 generat...

Wu Jiang et al, The Astrophysical Journal Letters 1000 2

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Phase-referenced images of GRS 1915+105 observe...

Phase-referenced images of GRS 1915+105 observed with EAVN at 6.7 GHz on 2023 April 15 (...

Wu Jiang et al, The Astrophysical Journal Letters 1000 2

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A region of the BOSS spectra (gray) for the fiv...

A region of the BOSS spectra (gray) for the five CEMP stars with the best-fit synthetic ...

Madeline Lucey et al, The Astrophysical Journal Letters 1000 2

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Distribution of sky positions (left panel), and...

Distribution of sky positions (left panel), and proper motions (right panel) in Magellan...

Madeline Lucey et al, The Astrophysical Journal Letters 1000 2

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The MINESweeper stellar parameters for our five...

The MINESweeper stellar parameters for our five CEMP stars (black stars) relative to the...

Madeline Lucey et al, The Astrophysical Journal Letters 1000 2

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The Galactocentric specific angular momentum in...

The Galactocentric specific angular momentum in the Lx–Lz plane for our five CEMP stars ...

Madeline Lucey et al, The Astrophysical Journal Letters 1000 2

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The absolute carbon abundance (A(C)) as a funct...

The absolute carbon abundance (A(C)) as a function of [Fe/H] for the five CEMP stars com...

Madeline Lucey et al, The Astrophysical Journal Letters 1000 2

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Carbon abundances ([C/Fe]) as a function of [Fe...

Carbon abundances ([C/Fe]) as a function of [Fe/H] for the five CEMP stars compared to l...

Madeline Lucey et al, The Astrophysical Journal Letters 1000 2

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The fits to the CH G band for the five CEMP sta...

The fits to the CH G band for the five CEMP stars. The black line with the gray shaded r...

Madeline Lucey et al, The Astrophysical Journal Letters 1000 2

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The fits to the Ca II infrared triplet for the ...

The fits to the Ca II infrared triplet for the five CEMP stars. The black line with the ...

Madeline Lucey et al, The Astrophysical Journal Letters 1000 2

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The metallicities derived from the Ca II triple...

The metallicities derived from the Ca II triplet compared to the MINESweeper metallicity...

Madeline Lucey et al, The Astrophysical Journal Letters 1000 2

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Same as Figure 8 but for the strongest C2 Swan ...

Same as Figure 8 but for the strongest C2 Swan band.

Madeline Lucey et al, The Astrophysical Journal Letters 1000 2

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Metallicity (﹩{\rm{log}}({\rm{O}}/{\rm{H}})+12﹩...

Metallicity (﹩{\rm{log}}({\rm{O}}/{\rm{H}})+12﹩) maps calculated for AGN-type regions, b...

D. Ł. Król et al, The Astrophysical Journal Letters 1000 2

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SLI map and diagram for Mrk 573. Left panel: SL...

SLI map and diagram for Mrk 573. Left panel: SLI map, with colors reflecting SLI values,...

D. Ł. Król et al, The Astrophysical Journal Letters 1000 2

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The inferred Galactic distribution of RRL as a ...

The inferred Galactic distribution of RRL as a GMM. The face-on distribution evaluated a...

Madeline Lucey et al, The Astronomical Journal 171 4

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