Possible CO clouds interacting with the SNRs G21.8-0.6 and G32.8-0.1
文献类型：会议论文
| 作者 | Jianjun Zhou1 ; Jarken Esimbek1; Xizheng Zhang2; Hongbo Zhang2
|
| 出版日期 | 2007 |
| 会议名称 | IAU Symposium 242 Astrophysical masers and their environments |
| 会议日期 | 2007-03-12 |
| 会议地点 | Alice Springs, central Australia |
| 通讯作者邮箱 | zhoujj@xao.ac.cn |
| 关键词 | ISM:clouds ISM: individual (G21.8-0.6 G32.8-0.1) ISM:molecules masers supernova remnants |
| 卷号 | 242 |
| 页码 | 66-67 |
| 通讯作者 | Jianjun Zhou |
| 英文摘要 | We have obtained the first CO(1-0) maps towards the SNRs G21.8-0.6 and G32.8-0.1, which are associated with OH 1720 MHz masers. Based on the morphological correspondence between the radio remnant and the CO cloud, and the velocity and position agreement between the OH maser and CO clouds, we tentatively suggest the clouds may be interacting with G21.8- 0.6 and G32.8-0.1. However, the shock-excited line broadening was not obvious for these two SNRs. We discuss the possible reasons for this. |
| 会议主办者 | IAU |
| 会议录 | Astrophysical Masers and their EnvironmentsProceedings IAU Symposium No. 242
 |
| 会议录出版者 | Cambridge University Press |
| 学科主题 | 恒星和恒星物理 |
| 会议录出版地 | Cambreidge, United Kingdom |
| 语种 | 英语 |
| ISSN号 | 1743-9213 |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/292]  |
| 专题 | 恒星形成与演化研究团组 新疆天文台_射电天文研究室 |
| 作者单位 | 1.National Astronomical Observatories/Urumqi Observatory, CAS, China, 40-5 South Beijing Road, Urumqi Xinjiang 830011, China 2.National Astronomical Observatories, CAS, China, 20A, Datun Road, Chaoyang Dis, Beijing 100012 |
| 推荐引用方式 GB/T 7714 | Jianjun Zhou,Jarken Esimbek,Xizheng Zhang,et al. Possible CO clouds interacting with the SNRs G21.8-0.6 and G32.8-0.1[C]. 见:IAU Symposium 242 Astrophysical masers and their environments. Alice Springs, central Australia. 2007-03-12. |
入库方式： OAI收割
来源：新疆天文台
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