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Updated: Jun 27, 2026

In Situ Monitoring of Diffusion of Guest Molecules in Porous Media Using Electron Paramagnetic Resonance Imaging
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在宿主星系中的分子气体中,有一颗具有红移z=6.42的类星体

Fabian Walter1, Frank Bertoldi, Chris Carilli

  • 1National Radio Astronomy Observatory, PO Box 0, Socorro, New Mexico 87801, USA. fwalter@nrao.edu

Nature
|July 25, 2003
PubMed
概括

这项研究检测到一氧化碳 (CO) 排放,一个分子的标志物,在一个类星体宿主星系在红移z=6.42. 这一发现揭示了早期宇宙中大量的分子气体,这对快速的星系进化至关重要.

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