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Spatially Extended P II 1.188 μm and Fe II 1.257 μm Emission Lines in a Nearby Seyfert Galaxy NGC1068 Observed with OAO/ISLE

机译:OAO / ISLE观测到的附近塞弗特星系NGC1068的空间扩展P II 1.188μm和Fe II 1.257μm发射线

摘要

We present J-band long-slit spectroscopic observation of NGC 1068 classified as a Seyfert 2 galaxy. J-band observations with OAO/ISLE provide clear detection of spatially extended [Fe II] 1.257 μm and [P II] 1.188 μm lines. We found that [Fe II] 1.257 μm/[P II] 1.188 μm increases with distance from a central continuum peak. Observed line ratios around the nucleus (continuum peak) are consistent with a typical value expected from photoionization models, while the ratios at 3"–4" (210–280 pc) east and west of the nucleus are slightly higher than this. In the off nucleus region of NGC 1068 we also found a possible association between [Fe II] 1.257 μm/[P II] 1.188 μm and the radio continuum. This suggests a mild contribution of shock ionization induced by a radio jet outside nucleus while photoionization by the central energy source is dominant near the nucleus.
机译:我们目前将N波段1068的J波段长缝光谱观测归类为Seyfert 2星系。用OAO / ISLE进行的J波段观测可以清楚地检测到空间延伸的[Fe II] 1.257μm和[P II] 1.188μm线。我们发现[Fe II] 1.257μm/ [P II] 1.188μm随着距中心连续峰的距离增加而增加。观察到的原子核周围的线比率(连续峰)与光电离模型所预期的典型值一致,而原子核东部和西部3“ –4”(210–280 pc)处的比率稍高于此值。在NGC 1068的核外区域,我们还发现[Fe II] 1.257μm/ [P II] 1.188μm与射电连续体之间可能存在关联。这表明由核外的射流引起的冲击电离的温和贡献,而中央能量源的电离在核附近占主导。

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