Spectral Modeling of SNe Ia Near Maximum Light: Probing the Characteristics of Hydrodynamical Models
Open Access
- 1 July 2006
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 645 (1) , 480-487
- https://doi.org/10.1086/504101
Abstract
We have performed detailed non-local thermodynamic equilibrium (NLTE) spectral synthesis modeling of two types of one-dimensional hydrodynamical models: the very highly parameterized deflagration model W7, and two delayed-detonation models. We find that, overall, both models do about equally well at fitting well-observed SNe Ia near maximum light. However, the Si II λ6150 feature of W7 is systematically too fast, whereas for the delayed-detonation models it is also somewhat too fast but significantly better than that of W7. We find that a parameterized mixed model does the best job of reproducing the Si II λ6150 line near maximum light, and we study the differences in the models that lead to better fits to normal SNe Ia. We discuss what is required of a hydrodynamical model to fit the spectra of observed SNe Ia near maximum light.Keywords
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This publication has 55 references indexed in Scilit:
- Comparative Direct Analysis of Type Ia Supernova Spectra. I. SN 1994DPublications of the Astronomical Society of the Pacific, 2005
- Type IIP Supernovae as Cosmological Probes: A Spectral-fitting Expanding Atmosphere Model Distance to SN 1999emThe Astrophysical Journal, 2004
- Direct Numerical Simulations of Type Ia Supernovae Flames. II. The Rayleigh‐Taylor InstabilityThe Astrophysical Journal, 2004
- Deflagrations and Detonations in Thermonuclear SupernovaePhysical Review Letters, 2004
- Direct Numerical Simulations of Type Ia Supernovae Flames. I. The Landau‐Darrieus InstabilityThe Astrophysical Journal, 2004
- The Rise Times of High- and Low-Redshift Type I[CLC]a[/CLC] Supernovae Are ConsistentThe Astronomical Journal, 2000
- Type Ia Supernovae: Observational OverviewPublished by Springer Nature ,1997
- Circumstellar H from SN 1994D and future Type Ia supernovae: an observational test of progenitor modelsMonthly Notices of the Royal Astronomical Society, 1996
- Accreting white dwarf models for the type I supernovae. IV The optical spectrum of a carbon-deflagration supernovaThe Astrophysical Journal, 1985
- The luminosity of type I supernovaeThe Astrophysical Journal, 1980