期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 345, 期 3, 页码 705-713出版社
OXFORD UNIV PRESS
DOI: 10.1046/j.1365-8711.2003.07006.x
关键词
galaxies : active; galaxies : general; galaxies : individual : PG1211+143; galaxies : Seyfert; X-rays : galaxies
We report on the analysis of a similar to60-ks XMM-Newton observation of the bright, narrow emission line quasar PG1211+143. Absorption lines are seen in both European Photon Imaging Camera and Reflection Grating Spectrometer spectra corresponding to H- and He-like ions of Fe, S, Mg, Ne, O, N and C. The observed line energies indicate an ionized outflow velocity of similar to24 000 km s(-1). The highest energy lines require a column density of N(H)similar to 5 x 10(23) cm(-2), at an ionization parameter of log xisimilar to 3.4. If the origin of this high-velocity outflow lies in matter being driven from the inner disc, then the flow is likely to be optically thick within a radius of similar to130 Schwarzschild radii, providing a natural explanation for the big blue bump (and strong soft X-ray) emission in PG1211+143.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据