ASCA OBSERVATIONS OF NGC-1068

被引：0
|
作者：
UENO, S
MUSHOTZKY, RF
KOYAMA, K
IWASAWA, K
AWAKI, H
HAYASHI, I
机构：
[1] NASA,GODDARD SPACE FLIGHT CTR,HIGH ENERGY ASTROPHYS LAB,GREENBELT,MD 20771
[2] NAGOYA UNIV,SCH SCI,DEPT ASTROPHYS,CHIKUSA KU,NAGOYA 46401,JAPAN
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 1994年 / 46卷 / 03期
关键词：
GALAXIES; INDIVIDUAL; (NGC-1068); SEYFERT-II; X-RAYS; SPECTRA;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
With the high sensitivity and spectral resolution of the ASCA satellite, we have discovered strong emission lines from the H-like and/or He-like ions of Ne, Mg, Si, and S as well as Fe L and confirmed the complex structure of Fe K line emission in the Seyfert II galaxy NGC 1068. The continuum emission above 3 keV exhibits rather flat shape with no evidence of low energy absorption. The overall X-ray spectrum can be well explained with a model involving starburst activity plus an obscured active galactic nucleus.
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页码：L71 / L75
页数：5
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