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(a) ALMA 1.3 mm dust continuum contours toward ...

(a) ALMA 1.3 mm dust continuum contours toward IRAS 18360 overlaid polarization intensit...

Shixian Mo et al, The Astronomical Journal 172 2

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(a) The SiO (J = 5-4) emission observed with th...

(a) The SiO (J = 5-4) emission observed with the ALMA and integrated from 85.8 to 100.6 ...

Shixian Mo et al, The Astronomical Journal 172 2

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Zoomed-in view of the blue rectangle area in Fi...

Zoomed-in view of the blue rectangle area in Figure 1. Contours show higher-resolution (...

Shixian Mo et al, The Astronomical Journal 172 2

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Upper panel: the magnetic field lines (black se...

Upper panel: the magnetic field lines (black segments) overplotted on the SiO (J = 5–4) ...

Shixian Mo et al, The Astronomical Journal 172 2

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Ratio of rotational energy to gravitational ene...

Ratio of rotational energy to gravitational energy βrot vs. core radius. Data for the so...

Shixian Mo et al, The Astronomical Journal 172 2

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Top panel: rotation curves for CH3OH(102,9–93,9...

Top panel: rotation curves for CH3OH(102,9–93,9) in IRAS 18360. The projected distance i...

Shixian Mo et al, The Astronomical Journal 172 2

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Top panel: contour map of the total (Stokes I) ...

Top panel: contour map of the total (Stokes I) dust emission and the magnetic field vect...

Shixian Mo et al, The Astronomical Journal 172 2

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Structure function for a center region of IRAS ...

Structure function for a center region of IRAS 18360. The measured angle dispersion is s...

Shixian Mo et al, The Astronomical Journal 172 2

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The rotation temperature map for CH3OH. Only th...

The rotation temperature map for CH3OH. Only the locations with significant measurements...

Shixian Mo et al, The Astronomical Journal 172 2

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Spatial distribution of the B-field-to-gravity ...

Spatial distribution of the B-field-to-gravity force ratio ΣB toward IRAS 18360. The con...

Shixian Mo et al, The Astronomical Journal 172 2

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iSHELL M2 spectra (RP ﹩\equiv ﹩ λ/Δλ ﹩\cong ﹩ 4...

iSHELL M2 spectra (RP ﹩\equiv ﹩ λ/Δλ ﹩\cong ﹩ 4.5 × 104) of CO and H2O in Comet 13P and ...

Michael A. DiSanti et al, The Planetary Science Journal 7 7

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(a–b). Nucleus-centered spectra of 13P in order...

(a–b). Nucleus-centered spectra of 13P in orders containing the lines of CH4 used in our...

Michael A. DiSanti et al, The Planetary Science Journal 7 7

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(a–b) Comet 13P CH4 residual spectra, represent...

(a–b) Comet 13P CH4 residual spectra, representing observed spectra after subtracting mo...

Michael A. DiSanti et al, The Planetary Science Journal 7 7

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Portions of 13P raw M2 difference frames (A–B) ...

Portions of 13P raw M2 difference frames (A–B) representing (a) the first ABBA sequence ...

Michael A. DiSanti et al, The Planetary Science Journal 7 7

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Abundance ratios and ±1σ uncertainties for six ...

Abundance ratios and ±1σ uncertainties for six trace species relative to H2O in 13P, tog...

Michael A. DiSanti et al, The Planetary Science Journal 7 7

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Excitation analysis for Comet 13P/Olbers. (a) L...

Excitation analysis for Comet 13P/Olbers. (a) Line-by-line nucleus-centered CO productio...

Michael A. DiSanti et al, The Planetary Science Journal 7 7

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Ratios among CO, CH4, and C2H6, the three most ...

Ratios among CO, CH4, and C2H6, the three most volatile species systematically targeted ...

Michael A. DiSanti et al, The Planetary Science Journal 7 7

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Comparison of the ODR fits to the M dwarfs (lar...

Comparison of the ODR fits to the M dwarfs (large circles) and FGK stars (small gray cir...

T. C. L. Trueman et al, The Astrophysical Journal 1005 2

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GCE predictions for the abundance ratios of ref...

GCE predictions for the abundance ratios of refractory elements. The GCE tracks are labe...

T. C. L. Trueman et al, The Astrophysical Journal 1005 2

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Comparison of M dwarf abundances for our benchm...

Comparison of M dwarf abundances for our benchmark sample consisting of surveys using th...

T. C. L. Trueman et al, The Astrophysical Journal 1005 2

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Posterior slope overlap probabilities for the v...

Posterior slope overlap probabilities for the values of α derived from the bootstrap fit...

T. C. L. Trueman et al, The Astrophysical Journal 1005 2

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Difference of the bulk rotation rate of the RZ ...

Difference of the bulk rotation rate of the RZ from the background frame rate, Ωrz − 1/2...

Loren I. Matilsky et al, The Astrophysical Journal 1005 2

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(a) Horizontally averaged differential rotation...

(a) Horizontally averaged differential rotation, ...

Loren I. Matilsky et al, The Astrophysical Journal 1005 2

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Scatter symbols: realized amplitude of ...

Loren I. Matilsky et al, The Astrophysical Journal 1005 2

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(a) Schematic of our three-dimensional spherica...

(a) Schematic of our three-dimensional spherical-shell simulation domain. The yellow reg...

Loren I. Matilsky et al, The Astrophysical Journal 1005 2

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