| Abstract | We present model atmospheres for the first week of SN 1987A, based on the luminosity and density/velocity structure from hydrodynamic models of Woosley. The models account for line blanketing, expansion, sphericity, and departures from LTE in hydrogen and helium and differ from previously published efforts because our models represent ab initio calculations, i.e., they contain essentially no free parameters. The formation of the UV spectrum is dominated by the effects of line blanketing. In the absorption troughs, the Balmer line profiles were fit well by our models, but the observed emissions are significantly stronger than predicted, perhaps due to clumping. The generally good agreement between our synthetic spectra and observations provides independent support for the overall accuracy of the hydrodynamic models of Woosley. We address the question of the accuracy of the Baade-Wesselink method in a detailed discussion of its approximations. While the application of the standard method produces a distance within an uncertainty of 20% in the case of SN 1987A, systematic errors up to a factor of 2 are possible, particularly if the precursor was a red supergiant. The key parameter that determines the systematic error of the method is the density/velocity structure, which can vary for each individual supernova. The supernova- based extragalactic distance scale is not yet precise enough to be of practical interest, owing to the large possible systematic error in the Hubble constant, H_0_ ~ 60^times 2^_divided by 2_ km s^-1^ Mpc^-1^. |
