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Scaling relations for the six H I disks presen...

Scaling relations for the six H I disks presented in this study. The points correspond ...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Effects of various steps of the synthetic H I ...

Effects of various steps of the synthetic H I imaging pipeline for the three less-popul...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Ratio of observable H I in the filtered image ...

Ratio of observable H I in the filtered image to observable H I in the smoothed image ...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Log histogram of H I column density (NHI) vers...

Log histogram of H I column density (NHI) versus velocity dispersion (σ) summed for the...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Ideal first moment maps (projected velocity com...

Ideal first moment maps (projected velocity component) for Tempest at various position a...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Evolution of how much H I emission in the CGM ...

Evolution of how much H I emission in the CGM is observable as a function of the minimu...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Same as Figure 2, but for the three more-popula...

Same as Figure 2, but for the three more-populated systems at 20 Mpc. These systems have...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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H I covering fraction (﹩{{ \mathcal L }}_{HI}﹩...

H I covering fraction (﹩{{ \mathcal L }}_{HI}﹩) as a function of impact parameter for t...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Corresponding position–velocity plots for the i...

Corresponding position–velocity plots for the ideal first moment maps shown in Figure 9....

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Same as Figure 5, but for the more-populated sy...

Same as Figure 5, but for the more-populated systems (Cyclone, Hurricane, and Squall) at...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Ratio of observable H I to total (ideal) in th...

Ratio of observable H I to total (ideal) in the CGM at various steps in the synthetic i...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Visualizations for observable H I for Tempest,...

Visualizations for observable H I for Tempest, Maelstrom, and Blizzard for all survey p...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Visualizations for observable H I for Cyclone,...

Visualizations for observable H I for Cyclone, Hurricane, and Squall for all survey par...

Cameron W. Trapp et al, The Astrophysical Journal 1005 2

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Average radial profiles of the three velocity c...

Average radial profiles of the three velocity components, vϕ (left panel), vr (middle le...

Francesco Sylos Labini and Roberto Capuzzo-Dolcetta, The Astrophysical Journal 1005 2

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Comparison of weighted and unweighted mean azim...

Comparison of weighted and unweighted mean azimuthal velocities 〈vϕ〉 as a function of Ga...

Francesco Sylos Labini and Roberto Capuzzo-Dolcetta, The Astrophysical Journal 1005 2

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Comparison of the azimuthal velocity distributi...

Comparison of the azimuthal velocity distributions vϕ for stars in the bin 9 < R < 11 kp...

Francesco Sylos Labini and Roberto Capuzzo-Dolcetta, The Astrophysical Journal 1005 2

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The rotation curves with error bars in the diff...

The rotation curves with error bars in the different six vertical slices for Rd = 4.5 kpc.

Francesco Sylos Labini and Roberto Capuzzo-Dolcetta, The Astrophysical Journal 1005 2

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Upper panel: Vertical acceleration and number o...

Upper panel: Vertical acceleration and number of stars contributing to the average in fu...

Francesco Sylos Labini and Roberto Capuzzo-Dolcetta, The Astrophysical Journal 1005 2

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(i) Contributions to the midplane rotation curv...

(i) Contributions to the midplane rotation curve vc(R, z = 0 kpc) of the stellar compone...

Francesco Sylos Labini and Roberto Capuzzo-Dolcetta, The Astrophysical Journal 1005 2

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Best fit of the NFW model to the rotation curve...

Best fit of the NFW model to the rotation curves (top panel) and corresponding behavior ...

Francesco Sylos Labini and Roberto Capuzzo-Dolcetta, The Astrophysical Journal 1005 2

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Best fit of the DM disk model to the rotation c...

Best fit of the DM disk model to the rotation curves (top panel) and corresponding behav...

Francesco Sylos Labini and Roberto Capuzzo-Dolcetta, The Astrophysical Journal 1005 2

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(a)–(d): Chandra images in the 0.5–8 keV energy...

(a)–(d): Chandra images in the 0.5–8 keV energy range. (e) and (f): XMM EPIC-pn image in...

Julia Ahlvind et al, The Astrophysical Journal 1005 2

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Magnetar evolution models compared with observa...

Magnetar evolution models compared with observational data. The black solid line shows t...

Julia Ahlvind et al, The Astrophysical Journal 1005 2

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Excluded pulsar/magnetar parameter space for th...

Excluded pulsar/magnetar parameter space for three cases: negligible ejecta absorption (...

Julia Ahlvind et al, The Astrophysical Journal 1005 2

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Corner plot of the MCMC run for B and P0. The b...

Corner plot of the MCMC run for B and P0. The black dashed lines in the top left and bot...

Julia Ahlvind et al, The Astrophysical Journal 1005 2

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