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OPTICAL ABSORPTION AND EMISSION BANDS OF SiC_2 IN CARBON STARS

机译:碳星中SiC_2的吸光和发射带

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摘要

Observations of the Merrill-Sanford bands of SiC_2 in the 4750-5050 A spectral region, seen in absorption in some carbon stars and in emission in IRAS 12311—3509, are reported. Vibrational band assignments based on recent laser-based laboratory electronic spectroscopy of this molecule constitute substantial revisions compared with earlier work. Vibrational hot bands are very strong when present in carbon stars, but were greatly weakened in T Mus for a time in 1994, indicating that the bands were then formed in a cooler region than that typical of carbon star photospheres. Emission bands of SiC_2, with intensities that are consistent with optical excitation of cool gas, appear in IRAS 12311-3509 which is probably a J-type carbon star occulted by a dusty disk so that the star is seen by reflection from material out of the plane of the disk.
机译:据报道,在一些碳星的吸收和在IRAS 12311-3509的发射中观察到了在4750-5050 A光谱区域内SiC_2的Merrill-Sanford谱带。与以前的工作相比,基于该分子基于激光的近期实验室电子光谱学的振动带分配构成了实质性的修订。当存在于碳星中时,振动热带非常强,但在1994年的T Mus中曾被大大减弱,这表明该带是在比碳星光球典型的凉爽区域形成的。 IRAS 12311-3509中出现了强度与冷气体的光激发相一致的SiC_2发射带,它可能是由尘埃盘掩盖的J型碳星,因此该星可以通过物质反射而看到。磁盘平面。

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