Shuo Kong Dataverse

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1 to 10 of 481 Results

CO in the Draco Nebula: The Atomic-Molecular Transition Jun 1, 2024 Kong, Shuo, 2024, "CO in the Draco Nebula: The Atomic-Molecular Transition", https://doi.org/10.7910/DVN/7DO6EP, Harvard Dataverse, V1 data for paper "CO in the Draco Nebula: The Atomic-Molecular Transition" by John H. Bieging and Shuo Kong
12CO_2to1_Draco.fits.gz Jun 1, 2024 - CO in the Draco Nebula: The Atomic-Molecular Transition Gzip Archive - 69.2 MB - MD5: c351d756a80b530486ab402066a8166f CO(2-1) PPV cube
Filament formation through collision-induced magnetic reconnection Mar 29, 2024 Kong, Shuo, 2021, "Filament formation through collision-induced magnetic reconnection", https://doi.org/10.7910/DVN/CXHWRR, Harvard Dataverse, V3 Data and figure files for the simulations in Kong et al. (2021, ApJ, 906, 80) and Kong et al. (2023, ApJS, 265, 58).
CMRfield.mpg Mar 29, 2024 - Filament formation through collision-induced magnetic reconnection MPEG Video - 16.1 MB - MD5: 94900c5c859c544f87c2cd0c36b173a4 A movie showing the filament formation via CMR. The simulation data is from the fiducial model from Kong et al. (2021, ApJ, 906, 80). Gas with densities above rho=1 (840 cm-3) is volume rendered so we see the dense gas in the collision midplane. The streamlines show magnetic fields. The random seeding is between x=-0.08 and x=0.08 (pc). The movie s...
B_H_4.tgz Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection Gzip Archive - 17.5 GB - MD5: 5f94083c5ecdce4397789668d5598599 Athena++ output files for the strong field model B_H (Model #4 in Table 1 of Kong et al. 2023)
B_L_3.tgz Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection Gzip Archive - 17.0 GB - MD5: d84eb9024278de72c34df567755ee296 Athena++ output files for the weak field model B_L (Model #3 in Table 1 of Kong et al. 2023)
eta_H_2.tgz Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection Gzip Archive - 17.1 GB - MD5: 35447229ffd1d4399ae8f04c5455718f Athena++ output files for the high-resistivity model eta_H (Model #2 in Table 1 of Kong et al. 2023)
eta_L_1.tgz Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection Gzip Archive - 17.3 GB - MD5: 69092fdc998c3cb45c344092b93e4dad Athena++ output files for the low-resistivity model eta_L (Model #1 in Table 1 of Kong et al. 2023)
MRCOL_0.tgz Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection Gzip Archive - 17.2 GB - MD5: 2eec7e89d20bb72d61bc953300c41805 Athena++ output files for the fiducial model MRCOL (Model #0 in Table 1 of Kong et al. 2023)
R2_H_8.tgz Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection Gzip Archive - 17.0 GB - MD5: c457cb75099fba4a02557ca2c270148b Athena++ output files for the larger radius model R2_H (Model #8 in Table 1 of Kong et al. 2023)

CO in the Draco Nebula: The Atomic-Molecular Transition

Jun 1, 2024

Kong, Shuo, 2024, "CO in the Draco Nebula: The Atomic-Molecular Transition", https://doi.org/10.7910/DVN/7DO6EP, Harvard Dataverse, V1

data for paper "CO in the Draco Nebula: The Atomic-Molecular Transition" by John H. Bieging and Shuo Kong

12CO_2to1_Draco.fits.gz

Jun 1, 2024 - CO in the Draco Nebula: The Atomic-Molecular Transition

Gzip Archive - 69.2 MB -

CO(2-1) PPV cube

Filament formation through collision-induced magnetic reconnection

Mar 29, 2024

Kong, Shuo, 2021, "Filament formation through collision-induced magnetic reconnection", https://doi.org/10.7910/DVN/CXHWRR, Harvard Dataverse, V3

Data and figure files for the simulations in Kong et al. (2021, ApJ, 906, 80) and Kong et al. (2023, ApJS, 265, 58).

CMRfield.mpg

Mar 29, 2024 - Filament formation through collision-induced magnetic reconnection

MPEG Video - 16.1 MB -

A movie showing the filament formation via CMR. The simulation data is from the fiducial model from Kong et al. (2021, ApJ, 906, 80). Gas with densities above rho=1 (840 cm-3) is volume rendered so we see the dense gas in the collision midplane. The streamlines show magnetic fields. The random seeding is between x=-0.08 and x=0.08 (pc). The movie s...

B_H_4.tgz

Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection

Gzip Archive - 17.5 GB -

Athena++ output files for the strong field model B_H (Model #4 in Table 1 of Kong et al. 2023)

B_L_3.tgz

Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection

Gzip Archive - 17.0 GB -

Athena++ output files for the weak field model B_L (Model #3 in Table 1 of Kong et al. 2023)

eta_H_2.tgz

Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection

Gzip Archive - 17.1 GB -

Athena++ output files for the high-resistivity model eta_H (Model #2 in Table 1 of Kong et al. 2023)

eta_L_1.tgz

Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection

Gzip Archive - 17.3 GB -

Athena++ output files for the low-resistivity model eta_L (Model #1 in Table 1 of Kong et al. 2023)

MRCOL_0.tgz

Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection

Gzip Archive - 17.2 GB -

Athena++ output files for the fiducial model MRCOL (Model #0 in Table 1 of Kong et al. 2023)

R2_H_8.tgz

Feb 24, 2023 - Filament formation through collision-induced magnetic reconnection

Gzip Archive - 17.0 GB -

Athena++ output files for the larger radius model R2_H (Model #8 in Table 1 of Kong et al. 2023)

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