1423 images found

Left: direct gas-phase O/H vs. z measured in 19...

Left: direct gas-phase O/H vs. z measured in 19 CECILIA galaxies. The color of the circl...

Noah S. J. Rogers et al, The Astrophysical Journal Letters 997 2

The N/O–O/H abundance trends in the CECILIA gal...

The N/O–O/H abundance trends in the CECILIA galaxies, local star-forming nebulae (gray d...

Noah S. J. Rogers et al, The Astrophysical Journal Letters 997 2

Emission in the spatial direction of the 2D NIR...

Emission in the spatial direction of the 2D NIRSpec data of the galaxy BX474. The profil...

Noah S. J. Rogers et al, The Astrophysical Journal Letters 997 2

Comparisons of Stokes I, linear polarization, a...

Comparisons of Stokes I, linear polarization, and EVPA (top, center, and bottom rows, re...

Joseph M. Michail et al, The Astrophysical Journal 997 2

Hydrogen recombination line measurements for tw...

Hydrogen recombination line measurements for two apertures, centered on Sgr A* (left) an...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

Continuum model (top left) and extinction law (...

Continuum model (top left) and extinction law (top right) derived from a fit to the spec...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

Dust distribution functions Ψ(T, τ9.8) for the ...

Dust distribution functions Ψ(T, τ9.8) for the Sgr A* pixel (left), the Mini-spiral (cen...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

15 GHz VLA image. The gray box indicates the re...

15 GHz VLA image. The gray box indicates the region used to model the Mini-spiral extinc...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

Posterior distribution of the optical depth law...

Posterior distribution of the optical depth law τ(λ) defined in Equation (1). Different ...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

Example of defringing using the factor-analysis...

Example of defringing using the factor-analysis approach for the λ = 19.057 μm recombina...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

Dust continuum models and derived extinction la...

Dust continuum models and derived extinction laws for different regions observed with JW...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

Best overall MIR extinction law. The blue curve...

Best overall MIR extinction law. The blue curve shows the continuum extinction shifted b...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

Spatial variation of the line-derived extinctio...

Spatial variation of the line-derived extinction values for the 5.129 μm and 5.908 μm hy...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

Spatial variation of the line-derived extinctio...

Spatial variation of the line-derived extinction values for all lines with S/N > 6. Pixe...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

Extinction correction applied to a bright state...

Extinction correction applied to a bright state of Sgr A*. The top panel shows a power-l...

Sebastiano D. von Fellenberg et al, The Astrophysical Journal 995 2

Relationship between the orbital elements and t...

Relationship between the orbital elements and the GW coordinate frame. The direction fro...

A. G. Abac et al, The Astrophysical Journal Letters 995 1

Compare the results of constructed SIDM halos w...

Compare the results of constructed SIDM halos with J0946+1006 observations in the parame...

Shubo Li et al, The Astrophysical Journal 994 2

The temporal evolution of the central density ρ...

The temporal evolution of the central density ρ0 (left panel) and velocity dispersion ν0...

Shubo Li et al, The Astrophysical Journal 994 2

The evolution of the 3D density profiles (left ...

The evolution of the 3D density profiles (left panel), the 2D projected surface density ...

Shubo Li et al, The Astrophysical Journal 994 2

The density and mass profiles of a core-collaps...

The density and mass profiles of a core-collapse SIDM halo with M200 = 1011 M⊙ (correspo...

Shubo Li et al, The Astrophysical Journal 994 2

The posterior distributions of M200, c200, and ...

The posterior distributions of M200, c200, and rt from the tNFW model fitting. In the 1D...

Shubo Li et al, The Astrophysical Journal 994 2

Median SHMRs from different studies. Colored cu...

Median SHMRs from different studies. Colored curves show best-fit relations from P. S. B...

Shubo Li et al, The Astrophysical Journal 994 2

Same format as Figure 2, but here we include th...

Same format as Figure 2, but here we include the best-fit tNFW profile from our mock len...

Shubo Li et al, The Astrophysical Journal 994 2

Left: the MGE fitting result for the density pr...

Left: the MGE fitting result for the density profile of the input SIDM halo. The 3D dens...

Shubo Li et al, The Astrophysical Journal 994 2

Same format as Figure 3: dashed curves show the...

Same format as Figure 3: dashed curves show the original evolutionary tracks, while soli...

Shubo Li et al, The Astrophysical Journal 994 2

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