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- W81497406 abstract "Toprobetheeffectsofthenuclearactivityonthehost galaxy, it is essential to disentangle the relative contribution of shockexcitationfromthatofphotoionization.Onemilestoneto- wards this goal is the ability to model the bowshock structures created by the interaction of radio ejecta with their surrounding medium. We have built a bowshock model based on TDA's one (Taylor, Dyson & Axon 1992) which was itself derived from an earlier work on Herbig-Haro objects. Since TDA's original model supplied the astronomers with only (Oiii)�5007 fluxes and profiles for various models of bowshocks, we undertook to include magnetic fields and to incorporate all of the atomic data tables of the code Mappings Ic for the computation of ionization states, cooling rates and line emissivities of the gas. This new model allows us to map line ratios and profiles of extragalactic bowshocks for all major lines of astrophysical in- terest. In this first paper, we present our model, analyse the gas behavior along the bowshock and give some examples of model results." @default.
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- W81497406 date "1997-06-01" @default.
- W81497406 modified "2023-09-23" @default.
- W81497406 title "MODELING EXTRAGALACTIC BOWSHOCKS. I. THE MODEL" @default.
- W81497406 hasPublicationYear "1997" @default.
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