The spectra of comet Arend-Roland (1956h) I. Medium-dispersion spectra

Mo Jing-er, C.Y. Fan
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Abstract

This is the first of two papers reporting the spectra of the Comet Arend-Roland (1956h) observed with the 82″ telescope at the McDonald Observatory, Texas, USA. In this paper we report the results of the analysis of two spectra, one in the rangeλλ3700Å − 4800Å. Having a dispersion of 36Å/mm and the other, λλ5100Å−6800Å having a dispersion of 72Å/mm. (The second paper deals with the polarization of emission lines of the comet). The spectra show a very strong solar continuum shifted to the red because of the Doppler effect, indicating that the comet is very dusty. From the lengths perpendicular to the dispersion of the continuum on the spectrogram, we estimated the linear dimension of the coma of the comet as 4.3 × 103km.

Arend-Roland彗星(1956h)的光谱
这是美国德克萨斯州麦克唐纳天文台82″望远镜观测到的Arend-Roland彗星(1956h)光谱的两篇论文中的第一篇。本文报告了两个光谱的分析结果,一个在rangeλλ3700Å−4800Å。分散度为36Å/mm,而另一个,λλ5100Å−6800Å分散度为72Å/mm。(第二篇论文是关于彗星发射线的极化)。光谱显示,由于多普勒效应,一个非常强烈的太阳连续体转移到红色,这表明彗星是非常多尘的。根据光谱图上连续体色散的垂直长度,我们估计彗星彗发的线性尺寸为4.3 × 103km。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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