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Integrated Near-infrared Band Strengths Of Solid Ch_4 And Its Mixtures With N_2

机译:固体Ch_4及其与N_2混合物的综合近红外谱带强度

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摘要

We studied icy CH_4 and its mixtures with N_2 (temperature 16-40 K), using near-IR transmittance spectroscopy (1.0-3.6 μm), and monitoring the film growth using interference patterns of two lasers. We measured peak position, full width at half-maximum, and strengths of the methane bands, and density and real refractive index of the icy films. Results confirm and extend but also partially contradict previous studies on similar mixtures. Experimental data can be applied to interpret observations of solar system (trans-Neptunian objects) and interstellar ices, where methane and nitrogen are believed to be present. We predict the optical depths of two methane NIR bands in the line of sight of some dense molecular clouds.
机译:我们使用近红外透射光谱(1.0-3.6μm)研究了冰冷的CH_4及其与N_2(温度16-40 K)的混合物,并使用两个激光的干涉图样监测膜的生长。我们测量了峰位置,半峰全宽,甲烷带的强度以及冰膜的密度和实际折射率。结果证实并扩大了范围,但也部分与先前对类似混合物的研究相矛盾。实验数据可以用于解释太阳系(海王星横穿天体)和星际冰的观测结果,据信其中存在甲烷和氮。我们在一些致密分子云的视线中预测了两个甲烷近红外波段的光学深度。

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