Metallicity Effects in Non-LTE Model Atmospheres of Type Ia Supernovae
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P. Nugent | D. Branch | E. Baron | P. Hauschildt | E. Lentz
[1] Type Ia supernovae and the Hubble constant , 1972, astro-ph/9801065.
[2] J. C. Wheeler,et al. Models for Type I supernovae - Partially incinerated white dwarfs , 1984 .
[3] D. Branch. The Optical Spectrum of a Carbon-Deflagration Supernova , 1985 .
[4] R. Harkness. A Comparison of Carbon Deflagration Models for SN la , 1991 .
[5] M. Phillips,et al. The Absolute Magnitudes of Type IA Supernovae , 1993 .
[6] David Branch,et al. Spectroscopic differences between supernovae of type Ia in early-type and in late-type galaxies , 1993 .
[7] P. Nugent,et al. Spectrum synthesis of the Type Ia supernovae SN 1992A and SN 1981B , 1995 .
[8] R. Harkness,et al. Gamma-Ray Transfer and Energy Deposition in Supernovae , 1995, astro-ph/9501005.
[9] M. Phillips,et al. The Absolute Luminosities of the Calan/Tololo Type Ia Supernovae , 1996, astro-ph/9609059.
[10] William Press,et al. A Precise Distance Indicator: Type Ia Supernova Multicolor Light-Curve Shapes , 1996, astro-ph/9604143.
[11] P. Hoeflich,et al. Explosion Models for Type IA Supernovae: A Comparison with Observed Light Curves, Distances, H 0, and Q 0 , 1996 .
[12] R. Ellis,et al. Measurements of the cosmological parameters omega and lambda from the first seven supernovae at z greater than or equal to 0.35 , 1996, astro-ph/9608192.
[13] P. Nugent,et al. Synthetic Spectra of Hydrodynamic Models of Type Ia Supernovae , 1996, astro-ph/9612044.
[14] D. Arnett,et al. Supernovae and Nucleosynthesis , 1996 .
[15] The effects of Fe II non-LTE on nova atmospheres and spectra , 1996, astro-ph/9601149.
[16] Peter H. Hauschildt,et al. Parallel Implementation of the PHOENIX Generalized Stellar Atmosphere Program. II. Wavelength Parallelization , 1996, astro-ph/9709238.
[17] Detailed Non-LTE Model Atmospheres for Novae during Outburst. I. New Theoretical Results , 1997, astro-ph/9707104.
[18] Peter H. Hauschildt,et al. Parallel implementation of the PHOENIX generalized stellar atmosphere program. II. Wavelength parallelization , 1998 .
[19] J. Wheeler,et al. Type Ia Supernovae: Influence of the Initial Composition on the Nucleosynthesis, Light Curves, and Spectra and Consequences for the Determination of ΩM and Λ , 1997, astro-ph/9709233.
[20] M. Phillips,et al. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant , 1998, astro-ph/9805201.
[21] P. H. Hauschildt,et al. Numerical solution of the expanding stellar atmosphere problem , 1998 .
[22] R. Ellis,et al. Measurements of $\Omega$ and $\Lambda$ from 42 high redshift supernovae , 1998, astro-ph/9812133.
[23] G. Sonneborn,et al. Direct Analysis of Spectra of the Type Ic Supernova SN 1994I , 1999, astro-ph/9906496.
[24] D. Branch,et al. Determination of the Hubble Constant Using a Two-Parameter Luminosity Correction for Type Ia Supernovae , 1999, astro-ph/9904347.
[25] R. Kirshner,et al. Spectral Models of the Type Ic Supernova SN 1994I in M51 , 1999, astro-ph/9907172.
[26] On the High-Velocity Ejecta of the Type Ia Supernova SN 1994D , 1999, astro-ph/9903333.