File:Tde-simulation.jpg
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English: Computer simulation of the tidal disruption of a one solar mass star by a one million solar mass supermassive black hole, performed using the Phantom general relativistic smoothed particle hydrodynamics code. The snapshot shows the star spaghettified into a long thin stream, which self-intersects due to relativistic precession, causing material to plunge towards the black hole and generate strong outflows which ultimately smother the black hole. |
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| Source | Own work |
| Author | Danieljamesprice |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 01:25, 30 August 2024 | | 3,840 × 2,160 (183 KB) | Danieljamesprice (talk | contribs) | Uploaded while editing "Tidal disruption event" on en.wikipedia.org |
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