File:Initial phase of turbulent molecular cloud collapse.jpg
Original file (797 × 800 pixels, file size: 127 KB, MIME type: image/jpeg)
Summary[edit | edit source]
The initial phase of the collapse: the turbulence organizes the gas into a network of filaments, and decays thereafter through shocks.
Licensing[edit | edit source]
| Description |
The initial phase of the collapse: the turbulence organizes the gas into a network of filaments, and decays thereafter through shocks. |
|---|---|
| Source |
The image appears on a website entitled, "FRAGMENTATION OF THE FIRST GASEOUS OBJECTS TO STARS" at url=https://ned.ipac.caltech.edu/level5/Sept06/Loeb/Loeb5.html. |
| Date |
May 2002 |
| Author |
Matthew Bate, University of Exeter |
| Rationale |
No free licensed or public domain alternatives known to exist to show the initial phase of the collapse of a turbulent molecular cloud in the present-day Universe: the turbulence organizes the gas into a network of filaments, and decays thereafter through shocks about 2002. |
| Permission |
Fair Use |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 02:26, 14 May 2017 | | 797 × 800 (127 KB) | Marshallsumter (discuss | contribs) | The initial phase of the collapse: the turbulence organizes the gas into a network of filaments, and decays thereafter through shocks. Category:Star-forming regions |
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