EVIDENCE FOR THE IMPORTANCE OF RESONANCE SCATTERING IN X-RAY EMISSION LINE PROFILES OF THE O STAR ζ PUPPIS

Maurice A. Leutenegger; Stanley P. Owocki; Steven M. Kahn; Frits B. S. Paerels

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EVIDENCE FOR THE IMPORTANCE OF RESONANCE SCATTERING IN X-RAY EMISSION LINE PROFILES OF THE O STAR ζ PUPPIS

机译：O星ζ泵的X射线发射线轮廓中共振散射的重要性的证据

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We fit the Doppler profiles of the He-like triplet complexes of O VII and N VI in the X-ray spectrum of the O star ζ Pup, using XMM-Newton RGS data collected over ～400 ks of exposure. We find that they cannot be well fit if the resonance and intercombination lines are constrained to have the same profile shape. However, a significantly better fit is achieved with a model incorporating the effects of resonance scattering, which causes the resonance line to become more symmetric than the intercombination line for a given characteristic continuum optical depth τ_*. We discuss the plausibility of this hypothesis, as well as its significance for our understanding of Doppler profiles of X-ray emission lines in O stars.

机译：我们使用在〜400 ks曝光时收集的XMM-Newton RGS数据，将O VII和N VI的He样三重态复合物的多普勒谱图拟合在O星ζPup的X射线光谱中。我们发现，如果将共振线和组合线限制为具有相同的轮廓形状，它们将无法很好地拟合。但是，通过结合了共振散射效应的模型，可以获得更好的拟合效果，对于给定的特征连续光学深度τ_*，该模型使共振线变得比组合线更对称。我们讨论了该假设的合理性，以及其对于我们理解O星X射线发射谱线的多普勒剖面的意义。

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《The Astrophysical journal》 |2007年第1pt1期|p.642-649|共8页
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Maurice A. Leutenegger; Stanley P. Owocki; Steven M. Kahn; Frits B. S. Paerels;
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1. EVIDENCE FOR THE IMPORTANCE OF RESONANCE SCATTERING IN X-RAY EMISSION LINE PROFILES OF THE O STAR ζ PUPPIS [J] . Maurice A. Leutenegger, Stanley P. Owocki, Steven M. Kahn, The Astrophysical journal . 2007,第1Pt1期

机译：O星ζ泵的X射线发射线轮廓中共振散射的重要性的证据
2. X-RAY EMISSION-LINE PROFILE MODELING OF O STARS: FITTING A SPHERICALLY SYMMETRIC! ANALYTIC WIND-SHOCK MODEL TO THE CHANDRA SPECTRUM OF ζ PUPPIS [J] . ROBAN H. KRAMER, DAVID H. COHEN, STANLEY P. OWOCKI The Astrophysical journal . 2003,第1aaParta1期

机译：O形星的X射线发射线轮廓建模：适合球对称！ ζ小牛CHANDRA谱的解析激波模型
3. X-Ray Emission-Line Profile Modeling of O Stars: Fitting a Spherically Symmetric Analytic Wind-Shock Model to the Chandra Spectrum of ζ Puppis [J] . Roban H. Kramer, David H. Cohen, Stanley P. Owocki The Astrophysical journal . 2003,第1期

机译：O形星的X射线发射线轮廓建模：将球对称解析风震模型拟合到ζPuppis的钱德拉光谱
4. The Delta Scuti Star Rho Puppis: the Perfect Target to Probe the Theory Predicting Solar-like Oscillations in Cool Delta Scuti Stars [C] . V. Antoci, G. Handler, F. Carrier, Los Alamos Series Pulsation Meetings . 2009

机译：Delta Scuti Star Rho Puppis：探测理论预测在酷三角洲Scuti恒星中的理论的完美目标
5. BCL::SAS - Small Angle X-ray / Neutron Scattering Profiles to Assist Protein Structure Prediction. [D] . Putnam, Daniel Kent. 2016

机译：BCL :: SAS-小角度X射线/中子散射曲线可协助蛋白质结构预测。
6. A customizable software for fast reduction and analysis of large X-ray scattering data sets: applications of the new DPDAK package to small-angle X-ray scattering and grazing-incidence small-angle X-ray scattering [O] . Gunthard Benecke, Wolfgang Wagermaier, Chenghao Li, -1

机译：可定制的软件用于快速减少和分析大型X射线散射数据集：新的DPDAK软件包在小角度X射线散射和掠入射小角度X射线散射中的应用
7. Evidence for the importance of resonance scattering in X-ray emission line profiles of the O star $\zeta$ Puppis [O] . Leutenegger, Maurice A., Owocki, Stanley P., Kahn, Steven M., 2007

机译：X射线发射中共振散射重要性的证据 O星$ \ zeta $ puppis的线条轮廓

EVIDENCE FOR THE IMPORTANCE OF RESONANCE SCATTERING IN X-RAY EMISSION LINE PROFILES OF THE O STAR ζ PUPPIS

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