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Interpreting observations of molecular outflow sources: the MHD shock code mhd_vode

机译:分子流出源的解释性观察:MHD冲击代码mhd_vode

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The planar MHD shock code mhd_vode has been developed in order to simulate both continuous (C) type shock waves and jump (J) type shock waves in the interstellar medium. The physical and chemical state of the gas in steady-state may also be computed and used as input to a shock wave model. The code is written principally in FORTRAN 90, although some routines remain in FORTRAN 77. The documented program and its input data are described and provided as supplementary material, and the results of exemplary test runs are presented. Our intention is to enable the interested user to run the code for any sensible parameter set and to comprehend the results. With applications to molecular outflow sources in mind, we have computed, and are making available as supplementary material, integrated atomic and molecular line intensities for grids of C- and J-type models; these computations are summarized in the Appendices.
机译:已经开发了平面MHD冲击代码mhd_vode,以模拟星际介质中的连续(C)型冲击波和跳跃(J)型冲击波。稳定状态下气体的物理和化学状态也可以计算出来,并用作冲击波模型的输入。该代码主要用FORTRAN 90编写,尽管某些例程仍保留在FORTRAN 77中。描述的程序及其输入数据作为补充材料进行了描述和提供,并给出了示例性测试运行的结果。我们的目的是使感兴趣的用户能够为任何明智的参数集运行代码并理解结果。考虑到分子流出源的应用,我们已经计算出C型和J型模型网格的原子和分子线积分强度,并将其作为补充材料来使用。这些计算总结在附录中。

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