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CAVITY OF MOLECULAR GAS ASSOCIATED WITH SUPERNOVA REMNANT 3C 397
文献类型：期刊论文
| 作者 | Jiang, Bing1; Chen, Yang1,2; Wang, Junzhi1,2; Su, Yang3; Zhou, Xin1 ; Safi-Harb, Samar4; DeLaney, Tracey5
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2010-04-01 |
| 卷号 | 712期号:2页码:1147-1156 |
| 关键词 | ISM: individual objects (3C 397 (G41.1-0.3)) ISM: molecules ISM: supernova remnants |
| ISSN号 | 0004-637X |
| 英文摘要 | 3C 397 is a radio and X-ray bright Galactic supernova remnant (SNR) with an unusual rectangular morphology. Our CO observation obtained with the Purple Mountain Observatory at Delingha, Qinghai Province, China reveals that the remnant is well confined in a cavity of molecular gas and embedded at the edge of a molecular cloud (MC) at the local standard of rest systemic velocity of similar to 32 km s(-1). The cloud has a column density gradient increasing from southeast to northwest, perpendicular to the Galactic plane, in agreement with the elongation direction of the remnant. This systemic velocity places the cloud and SNR 3C 397 at a kinematic distance of similar to 10.3 kpc. The derived mean molecular density (similar to 10-30 cm(-3)) explains the high volume emission measure of the X-ray emitting gas. A (12)CO line broadening of the similar to 32 km s(-1) component is detected at the westmost boundary of the remnant, which provides direct evidence of the SNR MC interaction and suggests multi-component gas there with dense (similar to 10(4) cm(-3)) molecular clumps. We confirm the previous detection of an MC at similar to 38 km s(-1) to the west and south of the SNR and argue, based on H I self-absorption, that the cloud is located in the foreground of the remnant. A list of Galactic SNRs presently known and suggested to be in physical contact with environmental MCs is appended in this paper. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | GAMMA-RAY EMISSION ; MHZ MASER EMISSION ; PULSAR-WIND NEBULA ; SNR PUPPIS-A ; X-RAY ; GALACTIC-CENTER ; IC 443 ; CASSIOPEIA-A ; MAGIC TELESCOPE ; CO OBSERVATIONS |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000275594600032 |
| 公开日期 | 2011-11-23 |
| 源URL | [http://159.226.72.40/handle/332002/1029]  |
| 专题 | 紫金山天文台_分子云与恒星形成研究团组 |
| 作者单位 | 1.Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China 2.Nanjing Univ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Peoples R China 3.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 4.Univ Manitoba, Dept Phys & Astron, Winnipeg, MB R3T 2N2, Canada 5.MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA |
| 推荐引用方式 GB/T 7714 | Jiang, Bing,Chen, Yang,Wang, Junzhi,et al. CAVITY OF MOLECULAR GAS ASSOCIATED WITH SUPERNOVA REMNANT 3C 397[J]. ASTROPHYSICAL JOURNAL,2010,712(2):1147-1156. |
| APA | Jiang, Bing.,Chen, Yang.,Wang, Junzhi.,Su, Yang.,Zhou, Xin.,...&DeLaney, Tracey.(2010).CAVITY OF MOLECULAR GAS ASSOCIATED WITH SUPERNOVA REMNANT 3C 397.ASTROPHYSICAL JOURNAL,712(2),1147-1156. |
| MLA | Jiang, Bing,et al."CAVITY OF MOLECULAR GAS ASSOCIATED WITH SUPERNOVA REMNANT 3C 397".ASTROPHYSICAL JOURNAL 712.2(2010):1147-1156. |
入库方式： OAI收割
来源：紫金山天文台
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