Discontinuous Galerkin finite element method for the continuum radiative transfer problem inside axis-symmetric circumstellar envelopes

Open Access

Fig. 4

Temperature profiles (left panels) and normalised SEDs (right panels) for the spherically symmetric envelope, with $τ_{v_{0}} = 1$ $\[\tau_{v_{0}}=1\]$ (blue curve) and $τ_{v_{0}} = 10^{2}$ $\[\tau_{v_{0}}=10^{2}\]$ (orange curve). The cross marks represent the solution from this study and the dashed curves are from DUSTY (Ivezic et al. 1997). The lower panels show the relative differences between the two codes.

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