The Milky Way Imaging Scroll Painting (MWISP): Project Details and Initial Results from the Galactic Longitudes of 25 degrees.8-49 degrees.7
文献类型:期刊论文
作者 | Su, Yang1,2; Yang, Ji1,2![]() ![]() ![]() ![]() ![]() |
刊名 | ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
![]() |
出版日期 | 2019 |
卷号 | 240期号:1页码:21 |
关键词 | Galaxy: structure ISM: clouds ISM: molecules radio lines: ISM stars: formation surveys |
ISSN号 | 0067-0049 |
DOI | 10.3847/1538-4365/aaf1c8 |
通讯作者 | Su, Yang(yangsu@pmo.ac.cn) |
英文摘要 | The Milky Way Imaging Scroll Painting project is an unbiased Galactic plane CO survey for mapping regions of l = -10 degrees to +250 degrees and vertical bar b vertical bar less than or similar to 5 degrees.2 with the 13.7 m telescope of the Purple Mountain Observatory. The legacy survey aims to observe the (CO)-C-12, (CO)-C-13, and (CO)-O-18 (J = 1-0) lines simultaneously with full-sampling using the nine-beam Superconducting SpectroScopic Array Receiver system with an instantaneous bandwidth of 1 GHz. In this paper, the completed 250 deg(2) data from l = +25 degrees.8 to +49 degrees.7 are presented with a grid spacing of 30 '' and a typical rms noise level of similar to 0.5 K for (CO)-C-12 at the channel width of 0.16 km s(-1) and similar to 0.3 K for (CO)-C-13 and (CO)-O-18 at 0.17 km s(-1). The high-quality data, with moderate resolution (similar to 50 ''), uniform sensitivity, and high spatial dynamic range, allow us to investigate the details of molecular clouds (MCs) traced by the three CO isotope lines. Three interesting examples are briefly investigated, including distant Galactic spiral arms traced by CO emission with V-LSR < 0 km s(-1), the bubble-like dense gas structure near the H II region W40, and the MCs distribution perpendicular to the Galactic plane. |
WOS关键词 | MOLECULAR CLOUDS ; CO SURVEY ; GAS ; PLANE |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000455131500006 |
出版者 | IOP PUBLISHING LTD |
源URL | [http://libir.pmo.ac.cn/handle/332002/19252] ![]() |
专题 | 中国科学院紫金山天文台 |
通讯作者 | Su, Yang |
作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210034, Jiangsu, Peoples R China 2.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210034, Jiangsu, Peoples R China 3.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany |
推荐引用方式 GB/T 7714 | Su, Yang,Yang, Ji,Zhang, Shaobo,et al. The Milky Way Imaging Scroll Painting (MWISP): Project Details and Initial Results from the Galactic Longitudes of 25 degrees.8-49 degrees.7[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2019,240(1):21. |
APA | Su, Yang.,Yang, Ji.,Zhang, Shaobo.,Gong, Yan.,Wang, Hongchi.,...&Jiang, Zhibo.(2019).The Milky Way Imaging Scroll Painting (MWISP): Project Details and Initial Results from the Galactic Longitudes of 25 degrees.8-49 degrees.7.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,240(1),21. |
MLA | Su, Yang,et al."The Milky Way Imaging Scroll Painting (MWISP): Project Details and Initial Results from the Galactic Longitudes of 25 degrees.8-49 degrees.7".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 240.1(2019):21. |
入库方式: OAI收割
来源:紫金山天文台
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。