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首页> 外文期刊>The Astrophysical journal >Markarian 1239: A Highly Polarized Narrow-Line Seyfert 1 Galaxy with a Steep X-Ray Spectrum and Strong Ne IX Emission*
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Markarian 1239: A Highly Polarized Narrow-Line Seyfert 1 Galaxy with a Steep X-Ray Spectrum and Strong Ne IX Emission*

机译:Markarian 1239:高偏振窄线赛弗1星系,具有陡峭的X射线光谱和强的Ne IX发射*

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We report the results of an XMM-Newton observation of the narrow-line Seyfert 1 galaxy Mrk 1239. This optically highly polarized AGN has one of the steepest X-ray spectra found in AGNs, with αX = +3.0 based on ROSAT PSPC data. The XMM-Newton EPIC pn and MOS data confirm this steep X-ray spectrum. The pn data are best fitted by a power law with a partial-covering absorption model suggesting two light paths between the continuum source and the observer, one indirect scattered one, which is less absorbed, and a highly absorbed direct light path. This result agrees with the wavelength-dependent degree of polarization in the optical/UV band. Residuals in the X-ray spectra of all three XMM-Newton EPIC detectors around 0.9 keV suggest the presence of an emission-line feature, most likely the Ne IX triplet. The detection of Ne IX and the nondetection of O VII/O VIII suggest a supersolar Ne/O ratio.
机译:我们报告了XMM-Newton观测到的窄线塞弗1星系Mrk 1239的结果。这种光学高度偏振的AGN具有AGN中发现的最陡的X射线光谱之一,基于ROSAT PSPC数据,αX= +3.0。 XMM-Newton EPIC pn和MOS数据证实了这种陡峭的X射线光谱。 pn数据最好通过幂定律与部分覆盖的吸收模型拟合,该模型建议在连续体源和观察者之间有两条光路,一个间接散射的光路(吸收较少)和高度吸收的直接光路。该结果与光学/ UV波段中取决于波长的偏振度一致。所有三个XMM-Newton EPIC探测器的X射线光谱在0.9 keV附近的残差表明存在发射线特征,很可能是Ne IX三重态。 Ne IX的检测和O VII / O VIII的未检测表明有超高的Ne / O比。

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