Global Model of the Interstellar Medium in our Galaxy with New Constraints on the Hot Gas Component
Global Model of the Interstellar Medium in our Galaxy with New Constraints on the Hot Gas Component
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DOI：
10.1086/305469
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发表时间：
1998-04
期刊：
影响因子：
--
通讯作者：
K. Ferrière
中科院分区：
文献类型：
--
作者：
K. Ferrière
我们根据最新的观测数据和星际介质（ISM）处于流体静力平衡的要求，对星际气体、宇宙线、磁场、引力场、超新星和超级气泡的银河分布进行了建模。我们的模型 ISM 将在另一篇论文中用于计算热星际气体成分的填充因子作为银河半径和高度的函数。
We model the Galactic distribution of the interstellar gas, cosmic rays, magnetic fields, gravitational field, supernovae, and superbubbles, based on the most recent observational data and on the requirement that the interstellar medium (ISM) be in hydrostatic equilibrium. Our model ISM will be used in a companion paper to compute the filling factor of the hot interstellar gas component as a function of Galactic radius and height.