Open AccessA mapping survey of massive CO cores
Author(s) -
Guan Xin,
Wu Yuefang,
Ju Binggang
Publication year - 2008
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2008.13937.x
Subject(s) - physics , astrophysics , observatory , core (optical fiber) , telescope , power law , optics , statistics , mathematics
We mapped 21 star‐forming regions with the 12 CO, 13 CO and C 18 O (1−0) lines using the 13.7‐m telescope of Purple Mount Observatory. This mapping survey resolved 53 13 CO cores, of which 22 are sourceless. We obtained the physical parameters of these cores. The relation between 13 CO linewidth and core size and that between column density and core size were analysed. The cores 00211+6549−1 and 22566+5830 were found to have outflows. Systematic V LSR shifts were detected in nine regions: 00211+6549, 00232+6437, 05168+3634, 19199+1358, 20160+3911, 22566+5830, 23042+6000, S146 and S270. Signatures of infall and cloud collision were found in regions 18507+0121 and 19199+1358, respectively. We studied the mass function of these 13 CO cores. The core masses range from 3.40 to 4.64 × 10 4 M ⊙ , and the core mass function is a power‐law distribution of index −0.82 ± 0.04 .