X-RAY-EMISSION AND REFLECTION IN AGNS

被引：0

作者：

NETZER, H ^{[1
]}

机构：

[1] TEL AVIV UNIV,WISE OBSERV,IL-69978 TEL AVIV,ISRAEL

来源：

MULTI-WAVELENGTH CONTINUUM EMISSION OF AGN | 1994年 / 159期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

X-ray spectra of many AGNs are dominated by strong absorption-like features at low (0.5-1 keV) energies. Recent progress in modeling AGNs indicate that pure X-ray absorption is unlikely to be observed and the contribution of emission and reflection must be significant. Several such models are shown and compared with what is likely to be observed by two X-ray experiments, ROSAT and ASCA. It is argued that X-ray colors may be useful diagnostic tools in analyzing such spectra.

引用

页码：213 / 216

页数：4

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