银纬8.6°富碳AGB星周围60 μm和100 μm远红外线空腔的研究

A. K. Gautam, B. Aryal
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引用次数: 0

摘要

本文讨论了远红外IRAS图中位于R.A. (J2000) =01h41m 01s和Dec (J2000) = 71004’00 9远红外环G125+09 6内的AGB星周围远红外空腔的尘埃环境。在R.A. (J2000) = 01h46m57.2s和DEC (J2000) = 71024 ' 57.1”处发现了一个腔状结构(大直径约2.55pc,小直径约0.77pc),距离恒星约220pc。研究了空腔内通量密度、粉尘色温、粉尘质量、视消度的分布。进一步研究了普朗克函数沿扩展和压缩方向的分布,尘埃色温沿大小直径平方方向的分布。尘埃色温在(19.7±1.25)K到(21.1±0.55)K之间,表明空腔是孤立的、稳定的。将讨论对结果的可能解释。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Study of a Far Infrared Cavity at 60 μm and 100 μm IRAS Map around the Carbon-Rich AGB Star at Galactic Latitude 8.6°
In this paper, we discussed about the dusty environment of the far infrared cavity around the AGB star located at R.A. (J2000) =01h41m 01s and Dec (J2000) = 71o 04’ 00 9, lying within far infrared loop G125+09 6 in the far infrared IRAS maps. A cavity like structure (major diameter ∼2.55pc & minor diameter ∼0.77pc) is found to lie at R.A. (J2000) = 01h46m57.2s and DEC (J2000) = 71o24’57.1”, located at a distance ∼ 220pc from the star. We studied the distribution of flux density, dust color temperature, dust mass, visual extinction in the cavity. We further studied the distribution Planck function along extension and compression, distribution of dust color temperature along square of the major and minor diameters. The dust color temperature is found to lie in the range (19.7±1.25) K to (21.1±0.55)K which shows the cavity is isolated and stable. A possible explanation of the results will be discussed.
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