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We use the MESA code to calculate the evolution...

We use the MESA code to calculate the evolutionary tracks of the 12 M ...

Zhuowen Li et al, The Astrophysical Journal Letters 975 1

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The upper part shows the entire formation proce...

The upper part shows the entire formation process from the triple to PMB to Gaia BH1. Th...

Zhuowen Li et al, The Astrophysical Journal Letters 975 1

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The distribution of orbital periods and eccentr...

The distribution of orbital periods and eccentricity for the core carbon-depleted PMB si...

Zhuowen Li et al, The Astrophysical Journal Letters 975 1

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An overlay of H2O maser spot positions and the ...

An overlay of H2O maser spot positions and the 21.9 GHz continuum image of the radio com...

Jack F. Gallimore et al, The Astrophysical Journal Letters 975 1

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Restored and naturally weighted Stokes I, Q, an...

Restored and naturally weighted Stokes I, Q, and U images of the five brightest H2O mase...

Jack F. Gallimore et al, The Astrophysical Journal Letters 975 1

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Linear polarization map of the H2O megamasers o...

Linear polarization map of the H2O megamasers of NGC 1068. The maser spots are plotted a...

Jack F. Gallimore et al, The Astrophysical Journal Letters 975 1

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(a)–(b) 10 minute averages of near-relativistic...

(a)–(b) 10 minute averages of near-relativistic electron intensities observed by EPD/EPT...

D. Lario et al, The Astrophysical Journal 975 1

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Schematic representation of the nominal interpl...

Schematic representation of the nominal interplanetary magnetic field configuration in t...

D. Lario et al, The Astrophysical Journal 975 1

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Heliographic coordinates of the HXR flares obse...

Heliographic coordinates of the HXR flares observed by STIX (magenta and teal triangles)...

D. Lario et al, The Astrophysical Journal 975 1

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From top to bottom: Time profiles of 0.23–0.32 ...

From top to bottom: Time profiles of 0.23–0.32 MeV nucleon−1 H (red), 3He (black), 4He (...

D. Lario et al, The Astrophysical Journal 975 1

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(a) 10 minute averages of the electron intensit...

(a) 10 minute averages of the electron intensities measured by the sunward apertures of ...

D. Lario et al, The Astrophysical Journal 975 1

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SDO/AIA 193 Å running difference images shortly...

SDO/AIA 193 Å running difference images shortly after the origin of the ion events #4 (a...

D. Lario et al, The Astrophysical Journal 975 1

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From top to bottom: (a) Intensity of the type I...

From top to bottom: (a) Intensity of the type III radio emissions detected by STA/SWAVES...

D. Lario et al, The Astrophysical Journal 975 1

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The same as Figure 7 but using SDO/AIA 304 Å ob...

The same as Figure 7 but using SDO/AIA 304 Å observations in panels (b).

D. Lario et al, The Astrophysical Journal 975 1

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(a) Electron spectrograms combining intensities...

(a) Electron spectrograms combining intensities collected by the sunward aperture of EPT...

D. Lario et al, The Astrophysical Journal 975 1

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SDO/AIA 193 Å image taken on 2022 November 11 a...

SDO/AIA 193 Å image taken on 2022 November 11 at 11:41 UT. At that time, NOAA ARs 13140 ...

D. Lario et al, The Astrophysical Journal 975 1

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Distributions of the time delays between electr...

Distributions of the time delays between electron SRTs and the onset of the associated (...

D. Lario et al, The Astrophysical Journal 975 1

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From top to bottom: Near-relativistic and relat...

From top to bottom: Near-relativistic and relativistic electron intensities, energetic p...

D. Lario et al, The Astrophysical Journal 975 1

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SDO/AIA 211 Å images for the EUV phenomena rela...

SDO/AIA 211 Å images for the EUV phenomena related to the origin of the ion events #1 (l...

D. Lario et al, The Astrophysical Journal 975 1

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Time evolution of (a) 46.7–86.6 keV electron in...

Time evolution of (a) 46.7–86.6 keV electron intensities measured in each one of the fou...

D. Lario et al, The Astrophysical Journal 975 1

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From left to right: SDO/HMI line-of-sight magne...

From left to right: SDO/HMI line-of-sight magnetograms, H α ...

D. Lario et al, The Astrophysical Journal 975 1

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Time evolution of (a) 46.15–85.7 keV electron i...

Time evolution of (a) 46.15–85.7 keV electron intensities measured by Wind/3DP binned in...

D. Lario et al, The Astrophysical Journal 975 1

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The same as Figure B1 but for the 45–85 keV ele...

The same as Figure B1 but for the 45–85 keV electrons measured by STA/SEPT.

D. Lario et al, The Astrophysical Journal 975 1

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CO brightness temperature maps for Cloud 378 at...

CO brightness temperature maps for Cloud 378 at various v LSR. The bla...

Rui-Zhi Li et al, The Astronomical Journal 168 5

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Morphological identification maps of selected s...

Morphological identification maps of selected strongly correlated dust-CO clouds. For ea...

Rui-Zhi Li et al, The Astronomical Journal 168 5

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