Latest Images

Left: stellar mass black holes (1M⊙–102M⊙) for...

Accretion-modified Stars in Accretion D...

Left: stellar mass black holes (1M⊙–102M⊙) form accretion-modified stars (AMSs) to deno...

The Astrophysical Journal Letters 911 1 L14

The Bondi explosion driven by the hyper-Eddingt...

Accretion-modified Stars in Accretion D...

The Bondi explosion driven by the hyper-Eddington accretion onto the black hole of the (...

The Astrophysical Journal Letters 911 1 L14

Spectral energy distributions (SEDs) of the Bon...

Accretion-modified Stars in Accretion D...

Spectral energy distributions (SEDs) of the Bondi explosion. Nonthermal emission from th...

The Astrophysical Journal Letters 911 1 L14

The NuSTAR FPMA (black) and FPMB (red) light cu...

The Inner Accretion Flow in the Resurge...

The NuSTAR FPMA (black) and FPMB (red) light curves of Mrk 817. The full 3–79 keV count ...

The Astrophysical Journal Letters 911 1 L12

Top: the NuSTAR (black) and Swift (red) spectra...

The Inner Accretion Flow in the Resurge...

Top: the NuSTAR (black) and Swift (red) spectra of Mrk 817, jointly fit with a simple po...

The Astrophysical Journal Letters 911 1 L12

Left: the NuSTAR (black) and Swift (red) spectr...

The Inner Accretion Flow in the Resurge...

Left: the NuSTAR (black) and Swift (red) spectra of Mrk 817. The spectra are fit with th...

The Astrophysical Journal Letters 911 1 L12

The Swift/XRT hardness curve of Mrk 817, coveri...

The Inner Accretion Flow in the Resurge...

The Swift/XRT hardness curve of Mrk 817, covering the mission periods with dense monitor...

The Astrophysical Journal Letters 911 1 L12

Spectra for PSR B1557−50. First panel: H I emis...

Tiny-scale Structure Discovered toward ...

Spectra for PSR B1557−50. First panel: H I emission scaled to match GASS in the directio...

The Astrophysical Journal Letters 911 1 L13

For two epoch observations (left: E1, right: E2...

Tiny-scale Structure Discovered toward ...

For two epoch observations (left: E1, right: E2). The H I emission spectrum ...

The Astrophysical Journal Letters 911 1 L13

Schematic description of our model. Left panel:...

Post-merger Jets from Supermassive Blac...

Schematic description of our model. Left panel: pre-merger disk winds launched from the ...

The Astrophysical Journal Letters 911 1 L15

Left panel: nonthermal energy spectra expected ...

Post-merger Jets from Supermassive Blac...

Left panel: nonthermal energy spectra expected for uncollimated post-merger jets from an...

The Astrophysical Journal Letters 911 1 L15

Detection horizons for multiwavelength detector...

Post-merger Jets from Supermassive Blac...

Detection horizons for multiwavelength detectors, e.g., SKA, VLA, EVLA, ALMA, HST, JWST,...

The Astrophysical Journal Letters 911 1 L15

Planetary system multiplicity distributions fro...

The Impact of Stellar Clustering on the...

Planetary system multiplicity distributions from the full Winter et al. (2020) sample. T...

The Astrophysical Journal Letters 911 1 L16

Orbital period demographics in field and overde...

The Impact of Stellar Clustering on the...

Orbital period demographics in field and overdensity systems for the full Winter et al. ...

The Astrophysical Journal Letters 911 1 L16

Cumulative distribution functions comparing the...

The Impact of Stellar Clustering on the...

Cumulative distribution functions comparing the orbital period ratios of adjacent planet...

The Astrophysical Journal Letters 911 1 L16

Ratio of single-to-multiple planet systems dete...

The Impact of Stellar Clustering on the...

Ratio of single-to-multiple planet systems detected with Kepler as a function of the pro...

The Astrophysical Journal Letters 911 1 L16

All data sets used within this study are from 2...

Source-dependent Properties of Two Slow...

All data sets used within this study are from 2019 March 31 at 00:00 UT to 2019 April 5 ...

The Astrophysical Journal 910 1 63

Magnetic field data on 2019 April 1 from 00:00–...

Source-dependent Properties of Two Slow...

Magnetic field data on 2019 April 1 from 00:00–12:00 UT, with a calm solar wind period s...

The Astrophysical Journal 910 1 63

Same as the previous figure but with only the d...

Source-dependent Properties of Two Slow...

Same as the previous figure but with only the data points from the calm solar wind inter...

The Astrophysical Journal 910 1 63

Top panel: total pressure ptot = 2nekBTc,e + pm...

Source-dependent Properties of Two Slow...

Top panel: total pressure ptot = 2nekBTc,e + pmag in black, along with the electron gas ...

The Astrophysical Journal 910 1 63

Left column: data for calm solar wind intervals...

Source-dependent Properties of Two Slow...

Left column: data for calm solar wind intervals only, in red for state 1 and in blue for...

The Astrophysical Journal 910 1 63

Core electron temperature Tc,e (in eV) scaled t...

Source-dependent Properties of Two Slow...

Core electron temperature Tc,e (in eV) scaled to 35.6 R⊙, provided by the plasma QTN spe...

The Astrophysical Journal 910 1 63

Electron “flux” ne(35.6 R⊙)Vp (in cm−2 s−1) pro...

Source-dependent Properties of Two Slow...

Electron “flux” ne(35.6 R⊙)Vp (in cm−2 s−1) provided by the plasma QTN spectrum measured...

The Astrophysical Journal 910 1 63

Top panel: Carrington map from SDO-AIA EUV obse...

Source-dependent Properties of Two Slow...

Top panel: Carrington map from SDO-AIA EUV observations on 2019 March 31 at 00:00 UT and...

The Astrophysical Journal 910 1 63

Left: samples of magnetic field lines from the ...

Source-dependent Properties of Two Slow...

Left: samples of magnetic field lines from the optimized PFSS magnetic field model with ...

The Astrophysical Journal 910 1 63

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