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THE 15-20 μm SPITZER SPECTRA OF INTERSTELLAR EMISSION FEATURES IN NGC 7023

机译:NGC 7023的星际发射特性的15-20μsSPITZER谱

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摘要

We present 15-20 μm long-slit spectra of NGC 7023 from the Infrared Spectrograph (IRS) on Spitzer. We observe recently discovered interstellar emission features at 15.9, 16.4, 17.0, 17.4, 17.8, and 18.9 μm, throughout the reflection nebula. The 16.4 μm emission feature peaks near the photodissociation front northwest of the star, as the aromatic emission features (AEFs) at 3.3,6.2, and 11.3 μm do. The 16.4 μm emission feature is thus likely related to the AEFs and radiates by nonequilibrium emission. The new 18.9 μm emission feature, by contrast, decreases monotonically with stellar distance. We consider candidate species for the 18.9 μm feature, including polycyclic aromatic hydrocarbons, fullerenes, and diamonds. We describe future laboratory and observational research needed to identify the 18.9 μm feature carrier.
机译:我们从Spitzer上的红外光谱仪(IRS)展示了NGC 7023的15-20μm长缝光谱。我们在整个反射星云中观察到最近发现的星际发射特征,分别为15.9、16.4、17.0、17.4、17.8和18.9μm。 16.3μm的发射特征峰在恒星西北的光解离前沿附近,正如3.3、6.2和11.3μm处的芳香族发射特征(AEF)一样。因此,16.4μm的发射特征可能与AEF有关,并通过非平衡发射而辐射。相比之下,新的18.9μm发射特征随恒星距离单调减小。我们考虑了18.9μm特征的候选物种,包括多环芳烃,富勒烯和钻石。我们描述了识别18.9μm特征载体所需的未来实验室和观察研究。

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