A (CO)-C-12, (CO)-C-13, and (CO)-O-18 survey of infrared dark clouds

作者：Du, Fujun^*; Yang, Ji

来源：Astrophysical Journal, 2008, 686(1): 384-398.

DOI：10.1086/591221

• dust
• extinction
• Galaxy : structure
• infrared : ISM
• radio lines : ISM
• stars : formation

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.

• 出版日期2008-10-10
• 单位中国科学院紫金山天文台