On the Spatial Distribution of $^{13}$CO Structures within $^{12}$CO Molecular Clouds
Lixia Yuan, Ji Yang, Fujun Du, Xunchuan Liu, Yang Su, Qing-Zeng Yan,, Xuepeng Chen, Yan Sun, Shaobo Zhang, Xin Zhou, and Yuehui Ma

TL;DR
This study analyzes the spatial distribution of $^{13}$CO structures within $^{12}$CO molecular clouds, revealing a universal angular separation and proposing a fundamental unit for cloud assembly and destruction.
Contribution
It introduces a statistical analysis of $^{13}$CO structures' distribution within $^{12}$CO clouds and suggests a universal separation scale relevant for cloud evolution.
Findings
Approximately 50% of angular separations are 3-7 arcmin.
Radial velocity separations mainly range from 0.3 to 2.5 km/s.
A scaling relation exists between cloud area and $^{13}$CO structure count.
Abstract
We look into the 2851 CO molecular clouds harboring CO structures to reveal the distribution of the projected angular separations and radial velocity separations between their internal CO structures. The projected angular separations are determined using the minimal spanning tree algorithm. We find that 50 of the angular separations fall in a narrow range of 3 - 7 arcmin with a median of 5 arcmin, and the corresponding radial velocity separations mainly range from 0.3 km s to 2.5 km s. The mean and standard deviation of the angular separations of the internal CO structures within CO clouds appear to be universal, independent of the CO cloud angular areas and the counts of their internal CO structures. We also reveal a scaling relation between the CO cloud angular area and its harbored…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Phase Equilibria and Thermodynamics · Spectroscopy and Laser Applications
