40-350 MICRON OBSERVATIONS OF GALACTIC SOURCES
40-350 MICRON OBSERVATIONS OF GALACTIC SOURCES
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40-350 微米银河源观测
DOI：
10.1086/153988
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发表时间：
1975
期刊：
影响因子：
--
通讯作者：
A. Moorwood
中科院分区：
文献类型：
--
作者：
I. Furniss;R. E. Jennings;A. Moorwood
报告了用气球载望远镜观测到的 31 个源的宽带 40--350 $mu$ 测量结果。除一个源外，所有源均已被识别为银河系 H ii 区域，其中约三分之一是光学可见的。这些物体包括 W3（三个分量）、W49、RCW 36、RCW 38 和 24 个源，位于 l/sup II/=327 度和 349 度之间的银河平面上。大多数这些来源以前从未在远红外线中观察到过。 W3 区域的等高线图显示了从主连续体组件延伸的发射臂。 (AIP)
Broad-band 40--350 $mu$ measurements are reported for 31 sources observed with a balloon-borne telescope. All but one of the sources have been identified with galactic H ii regions, of which about one-third are optically visible. The objects include W3 (three components), W49, RCW 36, RCW 38, and 24 sources lying along the galactic plane between l/sup II/=327degree and 349degree. Most of these sources have not previously been observed in the far-infrared. A contour map of the W3 region shows an emission arm extending from the main continuum component. (AIP)