Výtrysk plazmatu
Výtrysk plazmatu (anglicky astrophysical jet, česky relativistický či astrofyzický výtrysk) je výtrysk hmoty (plazmatu) pozorovaný v astronomii. Vyskytuje se u center galaxií a hvězd. Proud částic se často blíží rychlosti světla (relativistický výtrysk). Tvoří se tam Alfvénovy vlny.[1]
Reference
- ↑ CLAVIN, Whitney. Distant black hole wave twists like giant whip. phys.org [online]. 2015-07-10 [cit. 2022-01-19]. Dostupné online. (anglicky)
Externí odkazy
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Média použitá na této stránce
ESO Centaurus A LABOCA.jpg
Autor: ESO/WFI (Optical); MPIfR/ESO/APEX/A.Weiss et al. (Submillimetre); NASA/CXC/CfA/R.Kraft et al. (X-ray), Licence: CC BY 4.0
Colour composite image of Centaurus A, revealing the lobes and jets emanating from the active galaxy’s central black hole. This is a composite of images obtained with three instruments, operating at very different wavelengths. The 870-micron submillimetre data, from LABOCA on APEX, are shown in orange. X-ray data from the Chandra X-ray Observatory are shown in blue. Visible light data from the Wide Field Imager (WFI) on the MPG/ESO 2.2 m telescope located at La Silla, Chile, show the background stars and the galaxy’s characteristic dust lane in close to "true colour".
Autor: ESO/WFI (Optical); MPIfR/ESO/APEX/A.Weiss et al. (Submillimetre); NASA/CXC/CfA/R.Kraft et al. (X-ray), Licence: CC BY 4.0
Colour composite image of Centaurus A, revealing the lobes and jets emanating from the active galaxy’s central black hole. This is a composite of images obtained with three instruments, operating at very different wavelengths. The 870-micron submillimetre data, from LABOCA on APEX, are shown in orange. X-ray data from the Chandra X-ray Observatory are shown in blue. Visible light data from the Wide Field Imager (WFI) on the MPG/ESO 2.2 m telescope located at La Silla, Chile, show the background stars and the galaxy’s characteristic dust lane in close to "true colour".