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Updated: May 8, 2026

Hyperpolarized Xenon for NMR and MRI Applications
16:20

Hyperpolarized Xenon for NMR and MRI Applications

Published on: September 6, 2012

来自磁星的短暂脉冲无线电辐射

Fernando Camilo1, Scott M Ransom, Jules P Halpern

  • 1Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, New York 10027, USA. fernando@astro.columbia.edu

Nature
|August 25, 2006
PubMed
概括

异常X射线脉冲星 (AXP) 或磁星已经被证明可以发射无线电脉冲,这是这些天体的首次. 这一发现将磁星与普通脉冲星联系起来,并为研究它们的磁场和冠状云开辟了新的途径.

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