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A New Window to See Hidden Side of Magnetized Universe
The bent jet structures emitted from MRC 0600-399 as observed by the MeerKAT radio telescope (left) are well reproduced by the simulation conducted on ATERUI II (right). The nearby galaxy B visible in the left part of the MeerKAT image is not affecting the jet and has been excluded in the simulation. (Credit: Chibueze, Sakemi, Ohmura et al. (MeerKAT image); Takumi Ohmura, Mami Machida, Hirotaka Nakayama, 4D2U Project, NAOJ (ATERUI II image))
New observations and simulations show that jets of high-energy particles emitted from the central massive black hole in the brightest galaxy in galaxy clusters can be used to map the structure of invisible inter-cluster magnetic fields. These findings provide astronomers with a new tool for investigating previously unexplored aspects of clusters of galaxies.

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South Africa ,Acolumba ,Eastern Cape ,Japan ,Tokyo ,Northern Karoo ,South Africa General ,Haruka Sakemi ,Mami Machida ,Hirotaka Nakayama ,Takumi Ohmura ,Kyushu University ,University Of Tokyo Institute For Cosmic ,National Astronomical Observatory Of Japan ,Cray Research ,National Astronomical Observatory ,Cosmic Ray Research ,Square Kilometre Array ,Frica ,University Of Tokyo ,Research Fellow ,Supercomputer ,Simulation ,Black Hole ,University ,Radiation ,Collision ,Telescope ,Research ,Universe ,கொலம்பா ,கிழக்கு கேப் ,ஜப்பான் ,டோக்கியோ ,வடக்கு கரோ ,கையஶு பல்கலைக்கழகம் ,தேசிய வானியல் கண்காணிப்பு ஆஃப் ஜப்பான் ,தேசிய வானியல் கண்காணிப்பு ,அண்ட ராய் ஆராய்ச்சி ,சதுரம் கிலோமீடர் வரிசை ,

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