Time-dependent radiative transfer with PHOENIX(Corrigendum)

Abstract

where λ∞/λ = γ (1 + βμ) is the Doppler factor (Baron et al. 2012). In the original work the transformation of the timedependent term from frequency space to wavelength space was neglected. Thus, our discussion of Eqs. (24)–(27) should read: For an implementation of the time dependence in the radiative transfer itself, the spherical symmetric special relativistic radiative transfer equation (SSRTE) for expanding atmospheres (Hauschildt & Baron 1999) is extended so that the additional time-dependent term is given by [ γ (1 + βμ) ]−1 1 c ∂I ∂t (24)