Evidence for a variable far-infrared source in NGC 6334
Evidence for a variable far-infrared source in NGC 6334
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NGC 6334 中可变远红外源的证据
DOI：
10.1086/183061
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发表时间：
1979
期刊：
影响因子：
--
通讯作者：
E. Wright
中科院分区：
文献类型：
--
作者：
B. Mcbreen;G. Fazio;M. Stier;E. Wright
NGC 6334的位置是40- 250.. Mu..分辨率为1'的10米光度计。已探测到六个远红外辐射源。第二个最强的源在早期的可变远红外源中没有检测到。位于OH和H/sub 2/O脉泽源位置的新源是扩展的（0 '.7 FEHM），其热光度为1.9 × 10/sup 5/ L/sub sun/，许多代表了迄今未观测到的原恒星坍缩的瞬态阶段。
NGC 6334 has been mapped with a 40--250 ..mu..m photometer with 1' resolution. Six sources of far-infrared radiation have been detected. The second-strongest source was not detected in an earlier variable far-infrared source. The new source, located at the position of OH and H/sub 2/O maser sources, is extended (0'.7 FEHM) and has a bolometric luminosity of 1.9 x 10/sup 5/ L/sub sun/ and many represent a hitherto unobserved transient stage of protostellar collapse.