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Space–time evolution of Si IV from observations...

What Causes the High Apparent Speeds in...

Space–time evolution of Si IV from observations with the IRIS 1400 slit-jaw channel reve...

The Astrophysical Journal Letters 849 1 L7

Space–time evolution of Si IV from observations...

What Causes the High Apparent Speeds in...

Space–time evolution of Si IV from observations with the IRIS 1400 slit-jaw channel reve...

The Astrophysical Journal Letters 849 1 L7

Space–time evolution of a top view of Si IV (in...

What Causes the High Apparent Speeds in...

Space–time evolution of a top view of Si IV (in IRIS Data Numbers per second assuming th...

The Astrophysical Journal Letters 849 1 L7

Maps of temperature (top row), and Si IV 1402 Å...

What Causes the High Apparent Speeds in...

Maps of temperature (top row), and Si IV 1402 Å emissivity (bottom row) from our numeric...

The Astrophysical Journal Letters 849 1 L7

Maps of temperature (top row), and Si IV 1402 Å...

What Causes the High Apparent Speeds in...

Maps of temperature (top row), and Si IV 1402 Å emissivity (bottom row) from our numeric...

The Astrophysical Journal Letters 849 1 L7

Maps of Joule heating due to the ambipolar diff...

What Causes the High Apparent Speeds in...

Maps of Joule heating due to the ambipolar diffusion (top row), and current density (bot...

The Astrophysical Journal Letters 849 1 L7

Heating fronts in the simulated spicules propag...

What Causes the High Apparent Speeds in...

Heating fronts in the simulated spicules propagate with the Alfvén speed. The top shows ...

The Astrophysical Journal Letters 849 1 L7

Recovery of ...

Initial Mass Function Variability (or N...

Recovery of ﹩{({\text{}}{\rm{M}}/{\rm{L}})}_{* }﹩ from mock data as a function of S/N fo...

The Astrophysical Journal Letters 850 1 L14

(Upper panels) Comparison of best-fit models (g...

Initial Mass Function Variability (or N...

(Upper panels) Comparison of best-fit models (gray) and data in key wavelength regions f...

The Astrophysical Journal Letters 850 1 L14

IMF mismatch parameter plotted against [Fe/H] (...

Initial Mass Function Variability (or N...

IMF mismatch parameter plotted against [Fe/H] (left), [Mg/Fe], (middle), and σ (right) f...

The Astrophysical Journal Letters 850 1 L14

Comparison of ...

Initial Mass Function Variability (or N...

Comparison of ﹩{({\text{}}{\rm{M}}/{\rm{L}})}_{\mathrm{dyn}}﹩ (gray) to ...

The Astrophysical Journal Letters 850 1 L14

Left panel: the spectral region around the Ca, ...

Enrichment in r-process Elements from M...

Left panel: the spectral region around the Ca, Fe, Ba, and Y absorption lines for the 12...

The Astrophysical Journal Letters 850 1 L12

Top panel: observed Ba abundances vs. Fe abunda...

Enrichment in r-process Elements from M...

Top panel: observed Ba abundances vs. Fe abundances for the 12 Draco stars. Our results ...

The Astrophysical Journal Letters 850 1 L12

Top panel: the observed Eu ratios of our 12 Dra...

Enrichment in r-process Elements from M...

Top panel: the observed Eu ratios of our 12 Draco stars. Symbols are the same as those u...

The Astrophysical Journal Letters 850 1 L12

Orbit projection for an example BH-LC with ...

Revealing Black Holes with Gaia

Orbit projection for an example BH-LC with ﹩{M}_{\mathrm{BH}}=10\,{M}_{\odot }﹩, ...

The Astrophysical Journal Letters 850 1 L13

Two-dimensional probability dimension functions...

Revealing Black Holes with Gaia

Two-dimensional probability dimension functions (PDFs) for all of the BH-LCs in the MW i...

The Astrophysical Journal Letters 850 1 L13

Mean number of observable BH-LCs as a function ...

Revealing Black Holes with Gaia

Mean number of observable BH-LCs as a function of limiting G magnitude computed from 500...

The Astrophysical Journal Letters 850 1 L13

Distributions for the number of observable prop...

Revealing Black Holes with Gaia

Distributions for the number of observable properties of BH-LCs in the MW (thin and thic...

The Astrophysical Journal Letters 850 1 L13

(a) An example of the measured magnetic turbule...

Nature of Stochastic Ion Heating in the...

(a) An example of the measured magnetic turbulent spectrums and the measured spectral in...

The Astrophysical Journal Letters 850 1 L11

(a) Data distribution, (b) median values of the...

Nature of Stochastic Ion Heating in the...

(a) Data distribution, (b) median values of the scalar proton temperature, (c) proton te...

The Astrophysical Journal Letters 850 1 L11

Cross sections of Figures 2(a)–(c) along ...

Nature of Stochastic Ion Heating in the...

Cross sections of Figures 2(a)–(c) along ﹩{\beta }_{| | p}=0.2﹩, 1, and 2, respectively.

The Astrophysical Journal Letters 850 1 L11

Cross sections of the binned Tp data in the (...

Nature of Stochastic Ion Heating in the...

Cross sections of the binned Tp data in the (﹩{\epsilon }_{p},{V}_{\mathrm{SW}}﹩) space ...

The Astrophysical Journal Letters 850 1 L11

Schematic diagram of the New Horizons trajector...

Interstellar Pickup Ion Observations to...

Schematic diagram of the New Horizons trajectory (orange) compared with the Voyager (gre...

The Astrophysical Journal Supplement Series 233 1 8

Example of SWAP observations taken at ∼25.7 au,...

Interstellar Pickup Ion Observations to...

Example of SWAP observations taken at ∼25.7 au, colored-coded and annotated with the pri...

The Astrophysical Journal Supplement Series 233 1 8

Carrington rotation-averaged He photoionization...

Interstellar Pickup Ion Observations to...

Carrington rotation-averaged He photoionization rate at 1 au.

The Astrophysical Journal Supplement Series 233 1 8

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New Release of the Astronomy Image Explorer!

A new release of the AAS's Astronomy Image Explorer occurred on May 5, 2016.

This release updates the search and sorting features based on user feedback; adds links to videos and interactive figures in our Journal articles; provides a new way for publishers to add images to the AIE. Get in touch to hear more!