| CO Clouds around SNR G21.8-0.6 and G32.8-0.1 |
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| 引用本文： | Jian-Jun Zhou Xi-Zheng Zhang Hong-Bo Zhang Jarken Esimbek Ju-Yong Zhang Bing-Gang Ju. CO Clouds around SNR G21.8-0.6 and G32.8-0.1[J]. 中国天文和天体物理学报, 2007, 7(5): 705-711 |
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| 作者姓名： | Jian-Jun Zhou Xi-Zheng Zhang Hong-Bo Zhang Jarken Esimbek Ju-Yong Zhang Bing-Gang Ju |
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| 作者单位： | National Astronomical |
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| 摘 要： | We made the first CO(I—0) mapping to SNR G21.8-0.6 and SNR G32.8-0.1, both associated with OH 1720 MHz maser.Based on the morphological correspondence and velocity and position agreement between the radio remnant and the CO clouds,we tentatively identify the clouds that are respectively interacting with the two SNRs.
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| 关 键 词： | ISM clouds—ISM individual(G21.8-0.6 G32.8-0.1)—ISM molecules—masers—supernova remnants |
| 修稿时间： | 2004-12-14 |
CO Clouds around SNR G21.8-0.6 and G32.8-0.1 |
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| Jian-Jun Zhou,Xi-Zheng Zhang,Hong-Bo Zhang,Jarken Esimbek,Ju-Yong Zhang,Bing-Gang Ju. CO Clouds around SNR G21.8-0.6 and G32.8-0.1[J]. Chinese Journal of Astronomy and Astrophysics, 2007, 7(5): 705-711 |
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| Authors: | Jian-Jun Zhou Xi-Zheng Zhang Hong-Bo Zhang Jarken Esimbek Ju-Yong Zhang Bing-Gang Ju |
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| Abstract: | We made the first CO(1-0) mapping to SNR G21.8-0.6 and SNR G32.8-0.1, both associated with OH 1720MHz maser. Based on the morphological correspondence and velocity and position agreement between the radio remnant and the CO clouds, we tentatively identify the clouds that are respectively interacting with the two SNRs. |
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| Keywords: | ISM clouds - ISM individual (G21.8-0.6,G32.8-0.1) - ISM molecules - masers - supernova remnants |
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