INFRARED [FE II] EMISSION LINES FROM RADIATIVE ATOMIC SHOCKS

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
B. Koo, J. Raymond, Hyun-Jeong Kim
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引用次数: 14

Abstract

[Fe II] emission lines are prominent in the infrared (IR) and important as diagnostic tools for radiative atomic shocks. We investigate the emission characteristics of [Fe II] lines using a shock code developed by Raymond (1979) with updated atomic parameters. We rst review general characteristics of the IR [Fe II] emission lines from shocked gas, and derive their uxes as a function of shock speed and ambient density. We have compiled available IR [Fe II] line observations of interstellar shocks and compare them to the ratios predicted from our model. The sample includes both young and old supernova remnants in the Galaxy and the Large Magellanic Cloud and several Herbig-Haro objects. We nd that the observed ratios of the IR [Fe II] lines generally fall on our grid of shock models, but the ratios of some mid-IR lines, e.g., [Fe II] 35.35 μm=[Fe II] 25.99 m, [Fe II] 5.340 μm=[Fe II] 25.99 μm, and [Fe II] 5.340 μm=[Fe II] 17.94 m, are signicantly oset from our model grid. We discuss possible explanations and conclude that while uncertainties in the shock modeling and the observations certainly exist, the uncertainty in atomic rates appears to be the major source of discrepancy.
辐射原子冲击的红外[fe]发射线
[Fe II]发射线在红外(IR)中是突出的,作为放射性原子冲击的诊断工具是重要的。我们使用Raymond(1979)开发的具有更新原子参数的激波代码来研究[Fe II]线的发射特性。我们首先回顾了激波气体的IR [Fe II]发射谱线的一般特征,并推导了它们的谱线与激波速度和环境密度的关系。我们已经汇编了星际冲击的红外[铁II]线观测结果,并将它们与我们的模型预测的比率进行了比较。样本包括银河系、大麦哲伦星云和几个赫比格-哈罗天体中年轻和古老的超新星遗迹。研究发现,红外[Fe II]谱线的观测比值一般落在激波模型的网格上,但[Fe II] 35.35 μm=[Fe II] 25.99 m、[Fe II] 5.340 μm=[Fe II] 25.99 m、[Fe II] 5.340 μm=[Fe II] 17.94 m等中红外谱线的观测比值与模型网格有明显偏差。我们讨论了可能的解释,并得出结论,虽然激波模拟和观测中的不确定性确实存在,但原子速率的不确定性似乎是差异的主要来源。
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来源期刊
Journal of the Korean Astronomical Society
Journal of the Korean Astronomical Society 地学天文-天文与天体物理
CiteScore
1.30
自引率
10.00%
发文量
0
审稿时长
>12 weeks
期刊介绍: JKAS is an international scientific journal publishing papers in all fields of astronomy and astrophysics. All manuscripts are subject to the scrutiny of referees. Manuscripts submitted to JKAS must comply with the ethics policy of JKAS. Six regular issues are published each year on February 28, April 30, June 30, August 31, October 31, and December 31. One year''s issues compose one volume.
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