A Log‐Quadratic Relation for Predicting...

Correlation between a galaxy’s supermassive black hole mass and the shape parameter (i.e...

A Log‐Quadratic Relation for Predicting...

Left: Same as the data points in Fig. 1, but this time the optimal three‐parameter log‐q...

A Log‐Quadratic Relation for Predicting...

Central "massive compact object" mass vs. host galaxy Sérsic index n. Filled circles rep...

A Log‐Quadratic Relation for Predicting...

Predicted correlation between SMBH mass and the central B‐band surface brightness of the...

A Log‐Quadratic Relation for Predicting...

Major‐axis R‐band light profiles for three elliptical galaxies with directly measured SM...

A Log‐Quadratic Relation for Predicting...

Major‐axis light profile for the disk galaxy NGC 4564, the bulge of the edge‐on lenticul...

The Spitzer Survey of the Small Magella...

Spatial coverage of the S3MC data, overlaid on the Hα "parking lot camera" image of the ...

The Spitzer Survey of the Small Magella...

Source count histograms for the different Spitzer wave bands in black (bin size is 0.2 m...

The Spitzer Survey of the Small Magella...

Color composite of the S3MC mosaic for the IRAC 8.0, 4.5, and 3.6 μm wave bands, represe...

The Spitzer Survey of the Small Magella...

Details of Fig. 3 on four star‐forming regions. The sharp change in the MIR colors in th...

The Spitzer Survey of the Small Magella...

The 24 μm image of the southwest region of the SMC bar at 6﹩\arcsec﹩ resolution, and the...

The Spitzer Survey of the Small Magella...

The F8/F24 ratio in the southwest region of the SMC bar as a function of the F24/F70 rat...

The Spitzer Survey of the Small Magella...

Optical CMDs of the stars detected in the different bands of Spitzer for which optical c...

The Spitzer Survey of the Small Magella...

Spitzer infrared CMDs of the SMC. The wave band corresponding to the ordinate axis is in...

The Spitzer Survey of the Small Magella...

Same as Fig. 7, but now with different populations selected by the magnitude and color c...

The Spitzer Survey of the Small Magella...

Infrared CMDs, as in Fig. 8, with the different populations identified using the color s...

The Spitzer Survey of the Small Magella...

Distribution throughout the SMC of the different populations of sources selected using t...

The Spitzer Survey of the Small Magella...

Color‐color plots in the Spitzer and 2MASS wave bands. The color of the symbols is ident...

The Spitzer Survey of the Small Magella...

Average SEDs of the different populations described in the main text. The SEDs were obta...

On Pitch‐Angle Scattering Rates of Inte...

Diagram showing a newly injected pickup ion distribution in velocity space (spacecraft f...

On Pitch‐Angle Scattering Rates of Inte...

Dispersion relations for parallel‐propagating Alfvén waves are shown with two examples o...

On Pitch‐Angle Scattering Rates of Inte...

Parallel velocity of a helium PUI in resonance with outgoing Alfvén waves (in units of t...

On Pitch‐Angle Scattering Rates of Inte...

Diagram showing a hemispheric pickup ion velocity distribution in radial field (spacecra...

On Pitch‐Angle Scattering Rates of Inte...

SOHO CTOF helium energy flux velocity spectra averaged over times of indicated transvers...

On Pitch‐Angle Scattering Rates of Inte...

Best‐fit dimensionless hemispheric diffusion coefficient D vs. log of the transverse wav...

Origin of Solar Torsional Oscillations

(a) Differential rotation (solid contours correspond to faster rotation, dashed contours...

Origin of Solar Torsional Oscillations

Torsional oscillations produced by periodic perturbations at a fixed location. The left ...

Origin of Solar Torsional Oscillations

Influence of viscosity and meridional flow on the poleward propagation of zonal flow var...

Origin of Solar Torsional Oscillations

Snapshots of the torsional oscillations caused by mechanical forcing (left) and thermal ...

Origin of Solar Torsional Oscillations

Mechanical forcing of low‐latitude zonal flow variations. Panels (a) and (c) show the fo...