Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· Full Refereed Journal Article (PDF/Postscript)
· arXiv e-print (arXiv:1107.0009)
· References in the article
· Citations to the Article (19) (Citation History)
· Refereed Citations to the Article
· SIMBAD Objects (42)
· NED Objects (2)
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
Confronting 2D delayed-detonation models with light curves and spectra of Type Ia supernovae
Authors:
Blondin, Stéphane; Kasen, Daniel; Röpke, Friedrich K.; Kirshner, Robert P.; Mandel, Kaisey S.
Affiliation:
AA(Centre de Physique des Particules de Marseille (CPPM), Université Aix-Marseille, CNRS/IN2P3, 163 avenue de Luminy, 13288 Marseille Cedex 9, France), AB(Department of Physics, University of California at Berkeley, 366 LeConte, Berkeley, CA 94720, USA; Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA), AC(Universität Würzburg, Am Hubland, D-97074 Würzburg, Germany; Max-Planck-Institut für Astrophysics, Karl-Schwarzschild-Strasse 1, D-85741 Garching, Germany), AD(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA), AE(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA)
Publication:
Monthly Notices of the Royal Astronomical Society, Volume 417, Issue 2, pp. 1280-1302. (MNRAS Homepage)
Publication Date:
10/2011
Origin:
WILEY
Astronomy Keywords:
supernovae: general
Abstract Copyright:
© 2011 The Authors. Monthly Notices of the Royal Astronomical Society © 2011 RAS
DOI:
10.1111/j.1365-2966.2011.19345.x
Bibliographic Code:
2011MNRAS.417.1280B

Abstract

We compare models for Type Ia supernova (SN Ia) light curves and spectra with an extensive set of observations. The models come from a recent survey of 44 two-dimensional delayed-detonation models computed by Kasen et al., each viewed from multiple directions. The data include optical light curves of 251 SNe Ia, some of which have near-infrared observations, and 2231 low-dispersion spectra from the Center for Astrophysics, plus data from the literature. These allow us to compare a wide range of SN Ia models with observations for a wide range of luminosities and decline rates. The analysis uses standard techniques employed by observers, including MLCS2k2, SALT2 and SNooPy for light-curve analysis, and the Supernova Identification (SNID) code of Blondin & Tonry for spectroscopic comparisons to assess how well the models match the data. The ability to use the tools developed for observational data directly on the models marks a significant step forward in the realism of the models. We show that the models that match observed spectra best lie systematically on the observed width-luminosity relation. Conversely, we reject six models with highly asymmetric ignition conditions and a large amount (≳1 M&sun;) of synthesized 56Ni that yield poor matches to observed SN Ia spectra. More subtle features of the comparison include the general difficulty of the models to match the U-band flux at early times, caused by hot ionized ejecta that affect the subsequent redistribution of flux at longer wavelengths. The models have systematically higher velocities than the observed spectra at maximum light, as inferred from the Si II lambda6355 line. We examine ways in which the asymptotic kinetic energy of the explosion affects both the predicted velocity and velocity gradient in the Si II and Ca II lines. Models with an asymmetric distribution of 56Ni are found to result in a larger variation of photometric and spectroscopic properties with viewing angle, regardless of the initial ignition setup. We discuss more generally whether highly anisotropic ignition conditions are ruled out by observations, and how detailed comparisons between models and observations involving both light curves and spectra can lead to a better understanding of SN Ia explosion mechanisms.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)
  New!

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints