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Updated: Mar 28, 2026

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

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広い線で活動する銀河核は,狭い線で活動する銀河核よりも速く回転する

Wolfram Kollatschny1, Matthias Zetzl

  • 1Institut für Astrophysik, Universität Göttingen, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany. wkollat@astro.physik.uni-goettingen.de

Nature
|February 19, 2011
PubMed
まとめ

活発な銀河核 (AGN) の超大質量ブラックホールは,放射線の幅と形との新しい関係を示しています. この発見は,黒い穴の質量推定を精錬する,支配的なケプラーの回転と乱流を明らかにします.

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The representation of magnetic fields by magnetic field lines is very useful in visualizing the strength and direction of the magnetic field. Each of the magnetic field lines forms a closed loop. The field lines emerge from the north pole (N), loop around to the south pole (S), and continue through the bar magnet back to the north pole.
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