OH Survey along Sightlines of Galactic Observations of Terahertz C | |
Tang, Ningyu1,2; Li, Di1,2,3; Heiles, Carl4; Yue, Nannan1,2; Dawson, J. R.5,6,7; Goldsmith, Paul F.8; Krco, Marko1; McClure-Griffiths, N. M.9; Wang, Shen1,2; Zuo, Pei1,2 | |
刊名 | ASTROPHYSICAL JOURNAL |
2017-04-10 | |
卷号 | 839期号:1 |
关键词 | evolution ISM: clouds ISM: molecules |
英文摘要 | We have obtained OH spectra of four transitions in the (2)Pi(3/2) ground state, at 1612, 1665, 1667, and 1720 MHz, toward 51 sightlines that were observed in the Herschel project Galactic Observations of Terahertz C+. The observations cover the longitude range of (32 degrees, 64 degrees) and (189 degrees, 207 degrees) in the northern Galactic plane. All of the diffuse OH emissions conform to the so-called "Sum Rule" of the four brightness temperatures, indicating optically thin emission conditions for OH from diffuse clouds in the Galactic plane. The column densities of the H I "halos" N(H-I) surrounding molecular clouds increase monotonically with OH column density, N(OH), until saturating when N(H-I)= 1.0 x 10(21) cm(-2) and N(OH) >= 4.5 x 10(15) cm(-2), indicating the presence of molecular gas that cannot be traced by H I. Such a linear correlation, albeit weak, is suggestive of H (I) halos' contribution to the UV shielding required for molecular formation. About 18% of OH clouds have no associated CO emission (CO-dark) at a sensitivity of 0.07 K, but are associated with C+ emission. A weak correlation exists between C+ intensity and OH column density for CO-dark molecular clouds. These results imply that OH seems to be a better tracer of molecular gas than CO in diffuse molecular regions. |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | INTERSTELLAR DUST CLOUDS ; NARROW SELF-ABSORPTION ; DARK MOLECULAR GAS ; WARM NEUTRAL HALOS ; MILKY-WAY ; H-I ; EMISSION ; GALAXY ; HYDROXYL ; CORES |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000399122600004 |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/8389] |
专题 | 国家天文台_射电天文研究部 |
作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China 4.Univ Calif Berkeley, Dept Astron, 601 Campbell Hall 3411, Berkeley, CA 94720 USA 5.Macquarie Univ, Dept Phys & Astron, N Ryde, NSW 2109, Australia 6.Macquarie Univ, MQ Res Ctr Astron Astrophys & Astrophoton, N Ryde, NSW 2109, Australia 7.CSIRO Astron & Space Sci, Australia Telescope Natl Facil, POB 76, Epping, NSW 1710, Australia 8.CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA 9.Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia |
推荐引用方式 GB/T 7714 | Tang, Ningyu,Li, Di,Heiles, Carl,et al. OH Survey along Sightlines of Galactic Observations of Terahertz C[J]. ASTROPHYSICAL JOURNAL,2017,839(1). |
APA | Tang, Ningyu.,Li, Di.,Heiles, Carl.,Yue, Nannan.,Dawson, J. R..,...&Wang, Jun-Jie.(2017).OH Survey along Sightlines of Galactic Observations of Terahertz C.ASTROPHYSICAL JOURNAL,839(1). |
MLA | Tang, Ningyu,et al."OH Survey along Sightlines of Galactic Observations of Terahertz C".ASTROPHYSICAL JOURNAL 839.1(2017). |
个性服务 |
查看访问统计 |
相关权益政策 |
暂无数据 |
收藏/分享 |
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。
修改评论