Scales of Stability and Turbulence in the Molecular ISM
arxiv(2024)
摘要
From the archival data of the BU-FCRAO ^13 CO GRS, we measure the radial
profiles of column density and turbulent velocity dispersion from the centers
of molecular clouds outward into the surrounding diffuse molecular ISM.
Averaged across spatial scales, the profiles are consistent with turbulence
that is on average in hydrostatic equilibrium. We measure the turbulent kinetic
energy (KE) and the gravitational potential energy (GE) within and the pressure
energy (PE) outside the clouds. The distribution of the sum 2KE-|GE|-PE has a
mean near zero indicating approximate virial equilibrium. The average pressure
energy is consistent with estimates of the pressure of the multiphase ISM at
the Galactic mid-plane. If the dynamical time scale of the turbulence scales
with its crossing time, this apparent equilibrium may result from the rapid
virialization of the KE and GE with respect to changes in PE. In a snapshot,
the clouds appear to be in virial equilibrium within a confining pressure.
However, the duration of the equilibrium is approximately the crossing time. An
analysis of Larson's scaling relationships of line width and column density
finds no correlation. Tthe inference of constant column density with cloud size
is a misinterpretation of this lack of correlation.
更多查看译文
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要