首页> 外文期刊>The Astrophysical journal >THE DISCOVERY OF PHOTOSPHERIC PHOSPHORUS AND IRON IN THE FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER SPECTRUM OF THE HOT DA WHITE DWARF GD 394
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THE DISCOVERY OF PHOTOSPHERIC PHOSPHORUS AND IRON IN THE FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER SPECTRUM OF THE HOT DA WHITE DWARF GD 394

机译:热白光短波GD 394远紫外分光光度计光谱中光球磷和铁的发现

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摘要

We report the discovery of the photospheric P v 3s(~2S)-3p(~2P°) transitions and Fe Ⅲ 3d~6(~5D)-3d~5(~6S)4p(~5P°) transitions detected in the far-UV spectrum of the hot hydrogen-rich white dwarf GD 394. The spectrum was obtained with the Far Ultraviolet Spectroscopic Explorer using the large aperture. The spectrum covers a wavelength range of 910-1180 A at a resolution of λ/Δλ ~ 15,000. The presence of photospheric phosphorus and iron is the first firm detection of heavy elements other than silicon in the photosphere of GD 394. This detection confirms Extreme Ultraviolet Explorer observations, which show evidence of heavy elements in the photosphere of GD 394 with relatively low individual abundances. The spectrum reveals also a host of photospheric Si Ⅲ and Si Ⅳ features.
机译:我们报告发现了在探测到的光球P v 3s(〜2S)-3p(〜2P°)跃迁和FeⅢ3d〜6(〜5D)-3d〜5(〜6S)4p(〜5P°)跃迁的发现。富含氢的热白矮星GD 394的远紫外光谱。该光谱是通过使用大孔径的远紫外光谱浏览器获得的。光谱以λ/Δλ〜15,000的分辨率覆盖了910-1180 A的波长范围。光球中磷和铁的存在是第一个牢固检测GD 394光球中除硅以外的重元素的方法。该检测结果证实了Extreme Ultraviolet Explorer观测结果,这些观察结果表明GD 394光球中重元素的个体丰度较低。 。该光谱还揭示了许多光球SiⅢ和SiⅣ特征。

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