A (CO)-C-12, (CO)-C-13, and (CO)-O-18 survey of infrared dark clouds | |
Du, Fujun; Yang, Ji![]() | |
刊名 | ASTROPHYSICAL JOURNAL
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2008-10-10 | |
卷号 | 686期号:1页码:384-398 |
关键词 | dust extinction Galaxy : structure infrared : ISM radio lines : ISM stars : formation |
ISSN号 | 0004-637X |
英文摘要 | Infrared dark clouds (IRDCs) are extinction features against the Galactic infrared background, mainly in themid-infrared band. Recently they were proposed to be potential sites of massive star formation. In this work we have made a (CO)-C-12, (CO)-C-13, and (CO)-O-18 (J = 1 -> 0) survey of 61 IRDCs, 52 of which are in the first Galactic quadrant, selected from a catalog given by Simon and coworkers, while the others are in the outer Galaxy, selected by visually inspecting the MSX images. Detection rates in the three CO lines are 90%, 71%, and 62%, respectively. The distribution of IRDCs in the first Galactic quadrant is consistent with the 5 kpc molecular ring picture, while a slight trace of a spiral pattern is also noticeable, and needs to be further examined. The IRDCs have a typical excitation temperature of 10 K and typical column density of several 10(22) cm(-2). Their typical physical size is estimated to be several parsecs using angular sizes from the Simon catalog. Typical volume density and typical LTE mass are similar to 5000 cm(-3) and similar to 5000 M-circle dot, respectively. The IRDCs are in or near virial equilibrium. The properties of IRDCs are similar to those of star-forming molecular clumps, and they seem to be intermediate between giant molecular clouds and Bok globules; thus they may represent early stages of massive star formation. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | 1ST GALACTIC QUADRANT ; MOLECULAR CLOUDS ; CARBON-MONOXIDE ; DENSE CORES ; MILKY-WAY ; ROTATION CURVE ; COMPLEXES ; GALAXY ; EXTINCTION ; PRECURSORS |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000259822200030 |
公开日期 | 2011-12-29 |
内容类型 | 期刊论文 |
源URL | [http://159.226.72.40/handle/332002/1837] ![]() |
专题 | 紫金山天文台_分子云与恒星形成研究团组 |
作者单位 | Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China |
推荐引用方式 GB/T 7714 | Du, Fujun,Yang, Ji. A (CO)-C-12, (CO)-C-13, and (CO)-O-18 survey of infrared dark clouds[J]. ASTROPHYSICAL JOURNAL,2008,686(1):384-398. |
APA | Du, Fujun,&Yang, Ji.(2008).A (CO)-C-12, (CO)-C-13, and (CO)-O-18 survey of infrared dark clouds.ASTROPHYSICAL JOURNAL,686(1),384-398. |
MLA | Du, Fujun,et al."A (CO)-C-12, (CO)-C-13, and (CO)-O-18 survey of infrared dark clouds".ASTROPHYSICAL JOURNAL 686.1(2008):384-398. |
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