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Abundance ratios as a function of [Fe/H]. Solid...

Abundance ratios as a function of [Fe/H]. Solid green circles show the abundances inferr...

Randa Asa’d et al, The Astronomical Journal 167 6

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Left panel: color–magnitude diagram. The red po...

Left panel: color–magnitude diagram. The red points show the stars in the photometric ca...

Randa Asa’d et al, The Astronomical Journal 167 6

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Radial-velocity-distribution function for the c...

Radial-velocity-distribution function for the candidate member stars of NGC 1856. The ve...

Randa Asa’d et al, The Astronomical Journal 167 6

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Our inferred abundance ratios as a function of ...

Our inferred abundance ratios as a function of [Fe/H] excluding any results with the coe...

Randa Asa’d et al, The Astronomical Journal 167 6

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Our inferred abundance ratios as a function of ...

Our inferred abundance ratios as a function of T eff excluding any res...

Randa Asa’d et al, The Astronomical Journal 167 6

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Correlation between the mean of the abundances ...

Correlation between the mean of the abundances obtained in this work and by Asa’d et al....

Randa Asa’d et al, The Astronomical Journal 167 6

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The figure above displays the residuals of spec...

The figure above displays the residuals of spectral fits for 40 of the final 327 stars, ...

Randa Asa’d et al, The Astronomical Journal 167 6

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Illustration of Cluster NGC1856: Stars in blue ...

Illustration of Cluster NGC1856: Stars in blue represent those observed by the Hubble Sp...

Randa Asa’d et al, The Astronomical Journal 167 6

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The figure above displays the residuals of spec...

The figure above displays the residuals of spectral fits for the second set of 40 stars ...

Randa Asa’d et al, The Astronomical Journal 167 6

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The figure above displays the residuals of spec...

The figure above displays the residuals of spectral fits for the third set of 40 stars f...

Randa Asa’d et al, The Astronomical Journal 167 6

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The figure above displays the residuals of spec...

The figure above displays the residuals of spectral fits for the fourth set of 40 stars ...

Randa Asa’d et al, The Astronomical Journal 167 6

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The figure above displays the residuals of spec...

The figure above displays the residuals of spectral fits for the fifth set of 40 stars f...

Randa Asa’d et al, The Astronomical Journal 167 6

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The figure above displays the residuals of spec...

The figure above displays the residuals of spectral fits for the sixth set of 40 stars f...

Randa Asa’d et al, The Astronomical Journal 167 6

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The figure above displays the residuals of spec...

The figure above displays the residuals of spectral fits for the seventh set of 40 stars...

Randa Asa’d et al, The Astronomical Journal 167 6

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The figure above displays the residuals of spec...

The figure above displays the residuals of spectral fits for the last set of 47 stars fr...

Randa Asa’d et al, The Astronomical Journal 167 6

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Left panels: two examples of microlensing light...

Left panels: two examples of microlensing light curves due to FFPs in which the parallax...

Parisa Sangtarash and Sedighe Sajadian, The Astronomical Journal 167 6

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Similar to Figure 1. In these two short-duratio...

Similar to Figure 1. In these two short-duration microlensing light curves the parallax ...

Parisa Sangtarash and Sedighe Sajadian, The Astronomical Journal 167 6

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The light purple histograms are the normalized ...

The light purple histograms are the normalized distributions of some parameters due to a...

Parisa Sangtarash and Sedighe Sajadian, The Astronomical Journal 167 6

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Similar to Figure 3. In these two microlensing ...

Similar to Figure 3. In these two microlensing events the parallax-induced deviations ar...

Parisa Sangtarash and Sedighe Sajadian, The Astronomical Journal 167 6

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The fraction of simulated events due to FFPs th...

The fraction of simulated events due to FFPs that are affected by parallax as a percenta...

Parisa Sangtarash and Sedighe Sajadian, The Astronomical Journal 167 6

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Scatter plot of the relative deviation in the E...

Scatter plot of the relative deviation in the Einstein crossing time δ ...

Parisa Sangtarash and Sedighe Sajadian, The Astronomical Journal 167 6

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The correlation matrix between the relative dev...

The correlation matrix between the relative deviations in the lensing parameters (the fi...

Parisa Sangtarash and Sedighe Sajadian, The Astronomical Journal 167 6

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Sketch of how thermal creep and Knudsen compres...

Sketch of how thermal creep and Knudsen compressors work in an idealized equilibrium set...

Tetyana Bila et al, The Planetary Science Journal 5 5

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Thermal creep in a granular setting. If the top...

Thermal creep in a granular setting. If the top is capped, i.e., has a finite reservoir,...

Tetyana Bila et al, The Planetary Science Journal 5 5

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Thermal creep on Mars under insolation. Due to ...

Thermal creep on Mars under insolation. Due to the solid-state greenhouse effect, the to...

Tetyana Bila et al, The Planetary Science Journal 5 5

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