Latest Images
Left-hand panel: solar system giants with spin ...
The oblateness signals for various planet spin ...
Confirmed (filled circles) and candidate (open ...
Left-hand panel: intensity profiles across the ...
Theoretic stellar power spectra of a Kepler-167...
Constraints on the oblateness f⊥ and obliquity ...
Similar to Figure 6 but for f⊥ = 0.05. The dete...
Simulated light curves of a Kepler-167e-like pl...
Similar to Figure 6 but for f⊥ = 0.
Comparison of 2D distribution of A(V), R(V), an...
Continuation of Figure 1.
Correlation between R(V) and qPAH using stars t...
R(V) distribution of LMC and SMC is shown in th...
Quantitative comparison on the per-star basis b...
R(V) variation as a function of the mass accret...
The cosmic-ray spectra (upper panels) and the c...
The configuration of stellar associations in an...
Same as Figure 3 for a PeVatron in Upper Centau...
The distance from Earth to the cluster progenit...
The average dose rate experienced at ground lev...
The cosmic-ray spectrum (upper panels) and the ...
The solar neighborhood ISO distribution, withou...
Predicted distribution of ISOs with similar vel...
Slices through the continuous three-dimensional...
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