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Updated: May 6, 2026

Synthesis of 68Ga Core-doped Iron Oxide Nanoparticles for Dual Positron Emission Tomography /T1Magnetic Resonance Imaging
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NGC 1068の活発な核の中央の塵に満ちたトーラス

W Jaffe1, K Meisenheimer, H J A Röttgering

  • 1Leiden Observatory, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands. jaffe@strw.leidenuniv.nl

Nature
|May 7, 2004
PubMed
まとめ

インターフェロメトリックの中赤外線観測により,活性銀河核 (AGN) の塵の渦が初めて空間的に解明されました. この構造は,AGNの外観を理解するために不可欠であり,安定性を保つために継続的なエネルギー投入を必要とします.

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