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首页> 外文期刊>The Astrophysical journal >IONIZATION NEBULAE SURROUNDING CAL 83 AND OTHER SUPERSOFT X-RAY SOURCES
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IONIZATION NEBULAE SURROUNDING CAL 83 AND OTHER SUPERSOFT X-RAY SOURCES

机译:围绕CAL 83和其他SUPERSOFT X射线源的电离星云

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We present the results of an optical search for ionized gaseous nebulae surrounding luminous, "supersoft" X-ray sources in the Large and Small Magellanic Clouds. This relatively new and mysterious X-ray class has characteristic luminosities ~10~(37)-10~(38) ergs s~(-1) with effective temperatures in the range of 2-6 x 10~5 K. The presence of a large flux of UV and soft X-ray photons from these objects has led to predictions of bright optical emission lines from the local interstellar medium. One such object, CAL 83 in the LMC, was known to have an associated nebula, and we quantify here the asymmetry and luminosity of this remarkable nebula. Deep images were made using narrowband filters to isolate the emission lines of Ha and [O Ⅲ] (λ5007). In these emission lines, the nebula is detected out to distances as far as 25 pc from the central object, and the integrated luminosity in each line is of order ~100 solar luminosity. Model calculations of such nebulae for chemical abundances characteristic of the LMC indicate that ~1% of the X-ray luminosity of the central source is reprocessed into the nebular Hα and [O Ⅲ] λ5007 emission lines, from which we conclude that the time-averaged X-ray luminosity of the central source, CAL 83, is greater than 3 x 10~(37) ergs s~(-1). The bright inner nebula contains ~150 solar mass within 7.5 pc of CAL 83, which clearly indicates that the nebular material has its origin in the interstellar medium. In sharp contrast, there were null detections for nebulae associated with nine other luminous, supersoft X-ray sources in the LMC and SMC, with upper limits for the [O Ⅲ] luminosity that are a factor of ~10 below that for CAL 83. For eight of these latter sources, we conclude that either their time-averaged luminosity is substantially below that of CAL 83, or that the local interstellar medium is much less dense. The latter effect may be enhanced by expansion of the ionized nebula during the last several million years.
机译:我们提出了围绕麦哲伦星云的发光“超软” X射线源周围的离子化气态星云进行光学搜索的结果。这种相对较新且神秘的X射线类别的特征亮度为〜10〜(37)-10〜(38)ers s〜(-1),有效温度范围为2-6 x 10〜5K。来自这些物体的大量紫外线和软X射线光子通量导致对来自本地星际介质的明亮光发射线的预测。已知一个这样的物体,即LMC中的CAL 83,具有一个相关的星云,我们在此量化了这一非凡星云的不对称性和光度。用窄带滤光片分离出Ha和[OⅢ](λ5007)的发射线,从而得到深图像。在这些发射线中,星云被检测到距中心物体25 pc的距离,并且每条线中的综合光度约为太阳光度的约100。此类星云对LMC的化学丰度特征的模型计算表明,中心源的X射线光度的约1%被重新处理为星云Hα和[OⅢ]λ5007发射线,由此我们得出结论,时间-中心源CAL 83的平均X射线发光度大于3 x 10〜(37)ers s〜(-1)。明亮的内部星云在CAL 83的7.5 pc内包含约150太阳质量,这清楚地表明星云物质起源于星际介质。与之形成鲜明对比的是,在LMC和SMC中未检测到与其他9个超柔光X射线源相关的星云,[OⅢ]光度的上限比CAL 83的上限低约10倍。对于后面的八种光源,我们得出的结论是,它们的时间平均发光度明显低于CAL 83的发光度,或者本地星际介质的密度低得多。在过去的几百万年中,电离星云的膨胀可能会增强后一种效应。

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