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Individual Light Curve Fits of SN la and H0

Published online by Cambridge University Press:  12 April 2016

P. Höflich ,
E. Müller  and
A. Khoklov
P. Höflich
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
E. Müller
Affiliation:
Max Planck Institut für Astrophysik, Karl-Schwarzschild- Str. 1, D-8046 Garching, Germany
A. Khoklov
Affiliation:
Dept. of Astronomy, University of Texas, Austin, TX 78712, USA

Abstract

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In order to study the question whether the appearance of SNIa should be uniform from theoretical point of view, we present light curves (LC) for a broad variety of models using our elaborated LC scheme, including implicit LTE-radiation transport, expansion opacities, MC-γ transport, etc. For more details see Khokhlov (1991), Höflich et al. (1992), Höflich et al. (1993), Khokhlov et al. (1993), and Müller et al. (1993).

We consider a set of 19 SNIa explosion models, which encompass all currently discussed explosion scenarios. The set consists of three deflagration models (DF1, DF1MIX, W7 o), two detonation models (DET1, DET2 *), two delayed detonation models (N21, N32 •), detonations in low density white dwarfs (CO095, CO10, CO11 *), six pulsating delayed detonation models (PDD3, PDD5-9 Δ) and three tamped detonation models (DET2ENV2, DET2ENV4, DET2ENV6 Δ). We also included the widely-used deflagration model W7 of Nomoto et al. (1984)

Type
Observations of Supernovae and the Cosmic Distance Scale
Information
International Astronomical Union Colloquium , Volume 145: Supernovae and Supernova Remnants , 1996 , pp. 29 - 31
Copyright
Copyright © Cambridge University Press 1996

References

Höflich, P., Müller, E.; Khokhlov, A. 1992, A&A 259, 243 Google Scholar
Höflich, P., Müller, E.; Khokhlov, A. 1993, A&A 268, 411 Google Scholar
Khokhlov, A. 1991, A&A 246, 383 Google Scholar
Khokhlov, A., Müller, E., Höflich, P. 1993, A&A 270, 23 Google Scholar
Müller, E.; Höflich, P. A&A in press, MPA 709 Google Scholar
Nomoto, K., Thielemann, F.-K., Yokoi, K. 1984, ApJ 286, 644 Google Scholar