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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Publikašuvnnas:	Revista Mexicana de Astronomía y Astrofísica
Váldodahkkit:	Carl L. Gardner, Jeremiah R. Jones, Perry B. Vargas
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	Universidad Nacional Autónoma de México 2018
Fáttát:	Física, Astronomía y Matemáticas
Liŋkkat:	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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