Numerical simulation of the HH 30 astrophysical jet near its launch site
We simulate the surface brightness of the HH 30 astrophysical jet near its launch site in the forbidden O I, N II, and S II doublets by post-processing gas dynamical simulations of densities and temperatures, using spectral line emission data from the astrophysical spectral synthesis package Cloudy....
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Principais autores: | , , |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2018
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| Fag: | |
| Online adgang: | https://www.redalyc.org/articulo.oa?id=57171627004 https://www.redalyc.org/journal/571/57171627004/ https://www.redalyc.org/journal/571/57171627004/html/ https://www.redalyc.org/journal/571/57171627004/57171627004.epub https://www.redalyc.org/journal/571/57171627004/movil |
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