在普通无线电脉冲星的X射线频谱中的吸收特征

Oleg Kargaltsev1, Martin Durant, Zdenka Misanovic

  • 1Department of Astronomy, 222 Bryant Space Science Center, University of Florida, Gainesville, FL 32611, USA. kargaltsev@astro.ufl.edu

Science (New York, N.Y.)
|August 28, 2012
PubMed
概括

研究人员在典型的旋转动力脉冲星 (J1740+1000) 的X射线光谱中检测到吸收特征. 这一发现表明,在中子星中,光谱线可能比以前认为的更常见.

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