Latest Images

Distribution of global stellar parameters for a...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Distribution of global stellar parameters for all stars in the catalog. The dark blue ba...

The Astrophysical Journal Supplement Series 225 2 32

Representative spectra and our fits across the ...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Representative spectra and our fits across the range of our sample for the first quarter...

The Astrophysical Journal Supplement Series 225 2 32

Same as Figure 2 but for the second quarter of ...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Same as Figure 2 but for the second quarter of our wavelength regions.

The Astrophysical Journal Supplement Series 225 2 32

Same as Figures 2 and 3 but for the third quart...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Same as Figures 2 and 3 but for the third quarter of our wavelength regions.

The Astrophysical Journal Supplement Series 225 2 32

Same as Figures 2–4 but for the final quarter o...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Same as Figures 2–4 but for the final quarter of our wavelength regions.

The Astrophysical Journal Supplement Series 225 2 32

Relative element sensitivities (...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Relative element sensitivities (﹩{S}_{\epsilon }﹩) for increased abundance for all eleme...

The Astrophysical Journal Supplement Series 225 2 32

The left column shows uncorrected solar relativ...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

The left column shows uncorrected solar relative abundances ([ϵ/H]) for the subset of dw...

The Astrophysical Journal Supplement Series 225 2 32

Same as Figure 7 but for heavier elements and o...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Same as Figure 7 but for heavier elements and overall metallicity. The left column shows...

The Astrophysical Journal Supplement Series 225 2 32

Comparisons between our uncorrected solar relat...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Comparisons between our uncorrected solar relative abundances and those from literature ...

The Astrophysical Journal Supplement Series 225 2 32

Fit to the bottom 10th percentile of total rota...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Fit to the bottom 10th percentile of total rotational broadening (﹩v\sin i﹩ and ...

The Astrophysical Journal Supplement Series 225 2 32

We analyzed the solar spectrum using 20 asteroi...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

We analyzed the solar spectrum using 20 asteroid spectra (Section 2.2) and recovered the...

The Astrophysical Journal Supplement Series 225 2 32

The bulk of the comparison stars are from the S...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

The bulk of the comparison stars are from the SPOCS catalog (VF05), which uses an analys...

The Astrophysical Journal Supplement Series 225 2 32

Comparisons to temperatures from interferometri...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Comparisons to temperatures from interferometric diameter measurements had a scatter sev...

The Astrophysical Journal Supplement Series 225 2 32

Differences with temperatures determined from i...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Differences with temperatures determined from infrared flux measurements with uncertaint...

The Astrophysical Journal Supplement Series 225 2 32

Differences with temperatures determined from s...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Differences with temperatures determined from spectroscopic measurements with uncertaint...

The Astrophysical Journal Supplement Series 225 2 32

Comparison of [Fe/H] and ﹩\mathrm{log}g﹩ derive...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Comparison of [Fe/H] and ﹩\mathrm{log}g﹩ derived with microturbulence fixed to 0.85 km s...

The Astrophysical Journal Supplement Series 225 2 32

Distribution of photometric metallicities of a ...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Distribution of photometric metallicities of a selection of nearby stars from Ibukiyama ...

The Astrophysical Journal Supplement Series 225 2 32

We substituted MARCS atmosphere models for ATLA...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

We substituted MARCS atmosphere models for ATLAS models in our analysis procedure and co...

The Astrophysical Journal Supplement Series 225 2 32

After setting the offset at solar temperatures ...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

After setting the offset at solar temperatures to zero, we subtracted our fits from the ...

The Astrophysical Journal Supplement Series 225 2 32

Same as Figure 19 but for the heavier elements ...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Same as Figure 19 but for the heavier elements and overall metallicity.

The Astrophysical Journal Supplement Series 225 2 32

After correcting for trends in our abundance de...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

After correcting for trends in our abundance determinations, we again compare our abunda...

The Astrophysical Journal Supplement Series 225 2 32

Abundance ratios for stars with ﹩\mathrm{log}g﹩...

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Abundance ratios for stars with ﹩\mathrm{log}g﹩ > 4.0 after applying our abundance corre...

The Astrophysical Journal Supplement Series 225 2 32

Same as Figure 22 but for the heavier elements....

SPECTRAL PROPERTIES OF COOL STARS: EXTE...

Same as Figure 22 but for the heavier elements. The [Cr/Fe] ratios demonstrate both the ...

The Astrophysical Journal Supplement Series 225 2 32

Panel (a) shows a snapshot of the main sunspot ...

INTERFERENCE OF THE RUNNING WAVES AT LI...

Panel (a) shows a snapshot of the main sunspot of NOAA 12127 at the passband of −0.4 Å o...

The Astrophysical Journal 816 1 30

Panel (a) distribution of the narrowband oscill...

INTERFERENCE OF THE RUNNING WAVES AT LI...

Panel (a) distribution of the narrowband oscillation powers along slit 1 as shown in Fig...

The Astrophysical Journal 816 1 30

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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!