AN ADDITIONAL SOURCE OF GAS IONIZATION IN THE EXTENDED NARROW-LINE REGION OF NGC-1068

被引：0

作者：

NAZAROVA, LS ^{[1
]}

机构：

[1] MOSCOW MV LOMONOSOV STATE UNIV, STERNBERG ASTRON INST, MOSCOW 119899, RUSSIA

来源：

ASTRONOMY & ASTROPHYSICS | 1995年 / 299卷 / 02期

关键词：

GALAXIES; ACTIVE; INDIVIDUAL; (NGC; 1068); NUCLEI; SEYFERT;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The results of calculations of gas emission spectra with both central and extended sources of ionization have been compared to the ratio of line intensities observed in the extended narrow line region of NGC 1068. The origin of an extended structure of anomalous strength in the [OIII]lambda 5007 and [NeV]lambda 3425 lines found by Evans and Dopita (1986) and Bergeron et al. (1989) could be due to an additional stellar source of gas ionization located at a distance 1-2 kpc from the nucleus.

引用

页码：359 / 364

页数：6

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