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CO Clouds around SNR G21.8-0.6 and G32.8-0.1
作者姓名:Jian-Jun  Zhou  Xi-Zheng  Zhang  Hong-Bo  Zhang  Jarken  Esimbek  Ju-Yong  Zhang  Bing-Gang  Ju
作者单位:National Astronomical
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.

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
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.
Authors:Jian-Jun Zhou  Xi-Zheng Zhang  Hong-Bo Zhang  Jarken Esimbek  Ju-Yong Zhang  Bing-Gang Ju
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.
Keywords:ISM  clouds - ISM  individual (G21  8-0  6  G32  8-0  1) - ISM  molecules - masers - supernova remnants
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