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强远红外源中CO(1-0)谱线的新观测
引用本文:张海燕,孙锦,平劲松.强远红外源中CO(1-0)谱线的新观测[J].北京师范大学学报(自然科学版),1999,35(2):220-223.
作者姓名:张海燕  孙锦  平劲松
作者单位:北京师范大学天文学系
摘    要:利用紫金山天台13.7m射电望远镜对20个强IRAS远红外源(F100μm〉500Jy)进行了CO(1-0)的谱线观测,全部观测到CO发射,其中6个源为第1次观测到CO(1-0)谱线,在新观测的源中,5个可能有分子外向流,这些观测源的红外性质暗示出它们是仍深埋在分子云中的年轻星,显示出远红外源与分子云有关。

关 键 词:年轻星体  强远红外源  谱线  观测  一氧化碳分子
修稿时间:1999-01-20

强远红外源中CO(1-0)谱线的新观测
Zhang Haiyan, Sun Jin, Ping Jinsong.强远红外源中CO(1-0)谱线的新观测[J].Journal of Beijing Normal University(Natural Science),1999,35(2):220-223.
Authors:Zhang Haiyan  Sun Jin  Ping Jinsong
Abstract:The observations of CO(1- 0) line emission from 20 strong IRAS sources are made with the 13.7m telescope of Purple Mountain Observatory at Qinhai station. The result shows that all detected sources have CO emission. It includes first confirmed detection in CO for 6 far infrared sources, and 5 newly detected sources may have molecular outflows. According to the infrated properties of these sources , they are YSOs still deeply embeded in the clouds for which they formed, and far infrared sources are related with molecular clouds.
Keywords:YSOs  bright far infrared  sources  CO line emission
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