The column density structure of Orion A depicted by N-PDF  

作　　者：Yue-Hui Ma Hong-Chi Wang Chong Li Ji Yang 

机构地区：[1]Purple Mountain Observatory and Key Laboratory of Radio Astronomy,Chinese Academy of Sciences,Nanjing 210033,China [2]University of Chinese Academy of Sciences,Beijing 100049,China [3]School of Astronomy and Space Science,University of Science and Technology of China,Anhui 230026,China

出　　处：《Research in Astronomy and Astrophysics》2020年第4期139-155,共17页天文和天体物理学研究（英文版）

基　　金：supported by National Key R&D Program of China(2017YFA0402701);Key Research Program of Frontier Sciences of CAS(QYZDJSSW-SLH047);supports by the National Natural Science Foundation of China(Grant Nos.11503086 and 11503087)。

摘　　要：We have conducted a large-field simultaneous survey of 12 CO,13 CO and C18O J=1-0 emission toward the Orion A giant molecular cloud(GMC)with a sky coverage of4.4 deg2 using the Purple Mountain Observatory(PMO)-13.7 m millimeter-wavelength telescope.We use the probability distribution function of the column density(N-PDF)to investigate the distribution of molecular hydrogen in the Orion A GMC.The H2 column density,derived from the 13CO emission,of the GMC is dominated by a log-normal distribution in the range from4×1021 to1.5×1023 cm-2 with excesses both at the low-density and high-density ends.The excess of the low-density end is possibly caused by an extended and low-temperature(10 K)component with velocities in the range of 5-8 km s-1.Compared with the northern sub-regions,the southern sub-regions of the Orion A GMC contain less gas with column density in NH2>1.25×1022 cm-2.The dispersions of the N-PDFs of the sub-regions are found to correlate with the evolutionary stages of the clouds across the Orion A GMC.The structure hierarchy of Orion A GMC is explored with the DENDROGRAM algorithm,and it is found that the GMC is composed of two branches.All structures except one in the tree have virial parameters less than 2,indicating self-gravity is important on the spatial scales from0.3 to4 pc.Although power-laws and departures from lognormal distributions are found at the high-density end of N-PDFs for active star-forming regions,the N-PDFs of structures in the Orion A GMC are predominantly lognormal on scales from R0.4 to 4 pc.

关 键 词：ISM:clouds ISM:individual objects(Orion A) ISM:structure stars:formation surveys TURBULENCE 

分 类 号：P144[天文地球—天体物理]