, (V16O)

Charles A Bowesman1, Sergei N Yurchenko1, Jonathan Tennyson1

  • 1Department of Physics and Astronomy, University College London, London, UK.

Molecular physics
|November 20, 2024
PubMed
概括

科学家们开发了一种新的氧化物 (VO) 光谱模型,以改善其在热木星大气层中的检测. 这个模型解释了超细合,这对于精确的光谱分析和理解系外行星大气层至关重要.

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