Latest Images
Left: stellar mass black holes (1M⊙–102M⊙) for...
The Bondi explosion driven by the hyper-Eddingt...
Spectral energy distributions (SEDs) of the Bon...
The NuSTAR FPMA (black) and FPMB (red) light cu...
Top: the NuSTAR (black) and Swift (red) spectra...
Left: the NuSTAR (black) and Swift (red) spectr...
The Swift/XRT hardness curve of Mrk 817, coveri...
Spectra for PSR B1557−50. First panel: H I emis...
For two epoch observations (left: E1, right: E2...
Schematic description of our model. Left panel:...
Left panel: nonthermal energy spectra expected ...
Detection horizons for multiwavelength detector...
Planetary system multiplicity distributions fro...
Orbital period demographics in field and overde...
Cumulative distribution functions comparing the...
Ratio of single-to-multiple planet systems dete...
All data sets used within this study are from 2...
Magnetic field data on 2019 April 1 from 00:00–...
Same as the previous figure but with only the d...
Top panel: total pressure ptot = 2nekBTc,e + pm...
Left column: data for calm solar wind intervals...
Core electron temperature Tc,e (in eV) scaled t...
Electron “flux” ne(35.6 R⊙)Vp (in cm−2 s−1) pro...
Top panel: Carrington map from SDO-AIA EUV obse...
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