11 to 20 of 478 Results
Gzip Archive - 17.2 GB -
MD5: ba5c58f3062de9edb5083b348a61a291
Athena++ output files for the lower density model rho2_L (Model #5 in Table 1 of Kong et al. 2023) |
Gzip Archive - 17.2 GB -
MD5: 56c98208dbf1fd146c7a786aff21f073
Athena++ output files for the higher temperature model T_H (Model #10 in Table 1 of Kong et al. 2023) |
Gzip Archive - 17.2 GB -
MD5: 1cbaa5024c542c4320fcfaf46bae56fe
Athena++ output files for the lower temperature model T_L (Model #9 in Table 1 of Kong et al. 2023) |
Gzip Archive - 17.3 GB -
MD5: 74699d1c1e7a612661e07924f0664dad
Athena++ output files for the faster collision model vx_H (Model #12 in Table 1 of Kong et al. 2023) |
Gzip Archive - 17.2 GB -
MD5: 287f9cb5dc173a5f002cb6bae8c8b4d4
Athena++ output files for the slower collision model vx_L (Model #11 in Table 1 of Kong et al. 2023) |
Gzip Archive - 17.2 GB -
MD5: b166f867b134b644fe18c291607a1667
Athena++ output files for the faster shear model vz_H (Model #14 in Table 1 of Kong et al. 2023) |
Gzip Archive - 17.3 GB -
MD5: 17d188530bc9ea6451a7d47587ab6194
Athena++ output files for the slower shear model vz_L (Model #13 in Table 1 of Kong et al. 2023) |
GIF Image - 36.2 MB -
MD5: 326e26fa33dfe819e28a832b734a29ad
3D volume rendering of the CMR-filament at different time steps and projections. |
Mar 15, 2021 -
Evidence of Core Growth in the Dragon Infrared Dark Cloud: A Path for Massive Star Formation
Adobe PDF - 196.8 KB -
MD5: f2ae67cf37c6dc4e308a25193fd4f5f6
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Mar 15, 2021 -
Evidence of Core Growth in the Dragon Infrared Dark Cloud: A Path for Massive Star Formation
Adobe PDF - 196.1 KB -
MD5: 0188867a8099664002dcef3c7763aa0d
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