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16 - Aspherity effects in supernovae

Published online by Cambridge University Press:  11 August 2009

P. Höflich
Affiliation:
University of Texas, Austin, TX 78712, USA
C. Gerardy
Affiliation:
University of Texas, Austin, TX 78712, USA
R. Quimby
Affiliation:
University of Texas, Austin, TX 78712, USA
Peter Höflich
Affiliation:
University of Texas, Austin
Pawan Kumar
Affiliation:
University of Texas, Austin
J. Craig Wheeler
Affiliation:
University of Texas, Austin
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Summary

Abstract

We present a brief summary of asphericity effects in thermonuclear and core collapse supernovae (SN), and how to distinguish the underlying physics by their observable signatures. Electron scattering is the dominant process to produce polarization which is one of the main diagnostical tools. Asphericities result in a directional dependence of the luminosity which has direct implications for the use of SNe in cosmology. For core collapse SNe, the current observations and their interpretations suggest that the explosion mechanism itself is highly aspherical with a well defined axis and, typically, axis ratios of 2 to 3. Asymmetric density/chemical distributions and off-center energy depositions have been identified as crucial for the interpretation of the polarization P. For thermonuclear SNe, polarization turned out to be an order of magnitude smaller strongly supporting rather spherical, radially stratified envelopes. Nevertheless, asymmetries have been recognized as important signatures to probe A) for the signatures of the progenitor system, B) the global asymmetry with well defined axis, likely to be caused by rotation of an accreting white dwarf or merging WDs, and C) possible remains of the deflagration pattern.

Introduction

During the last decade, advances in observational, theoretical and computational astronomy have provided new insights into the nature and physics of SNe and gamma-ray bursts. Due to the extreme brightness of these events, they are expected to continue to play important role in cosmology. SNe Ia allowed good measurements of the Hubble constant both by statistical methods and theoretical models.

Type
Chapter
Information
Cosmic Explosions in Three Dimensions
Asymmetries in Supernovae and Gamma-Ray Bursts
, pp. 142 - 150
Publisher: Cambridge University Press
Print publication year: 2004

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References

Cropper, M., Bailey, J., McCowage, J., Cannon, R., Couch, W. 1988, MNRAS 231, 685
Fesen, R. A. & Gunderson, K. S. 1996, ApJ, 470, 967CrossRef
Fisher, A., Branch, D., Nugent, P., Baron, E. 1997, 481L, 89
Gerardy, C., Höflich, P., Quimby, R., Wang, L. + the HET-SN team 2003, ApJ, submitted
Hatano, K., Branch, D., Lentz, E. J., Baron, E., Filippenko, A. V., Garnavich, P. 2000, ApJ 543, L94CrossRef
Hillebrandt, W., Niemeyer, J. 2000, ARAA 38, 191CrossRef
Höflich, P. 1991 A&A 246, 481
Höflich, P. 1995, ApJ 443, 89CrossRef
Höflich, P., Wheeler, J. C., Hines, D., Trammell, S. 1995, ApJ 459, 307CrossRef
Höflich, P., Khokhlov, A., Wang, L., 2002, AIP-Publ. 586, p. 459 & astro-ph/0104025
Höflich, P., Gerardy, C., Linder, E., & Marion, H. 2003, in: Stellar Candles, eds. Gieren et al., Lecture Notes in Physics, Springer Press, in press & astro-ph/0301334
Howell, A., Höflich, P., Wang, L., Wheeler, J. C. 2001, ApJ 556, 302CrossRef
Jeffrey, D. J., 1991, ApJ, 375, 264CrossRef
Kasen, D., Nugent, P., Wang, L., Howell, A., Wheeler, J. C., Höflich, P., Baade, D., Baron, E., Hauschildt, P. 2003, ApJ, in press & astro-ph/0301312
Khokhlov, A. 2001, astro-ph/0008463
Leonard, D. C., Filippenko, A. V., Barth, A. J., Matheson, T. 2000, ApJ 536, 239CrossRef
Mendez, R. H.et al. 1977, ApJ 334, 295CrossRef
Scheck, L., Plewa, T., Janka, H.-T., Kifonidis, K., Müller, E. 2003, Phys. Rev. Let, submitted
Strom, R., Johnston, H. M., Verbunt, F., Aschenbach, B. 1995, Nature, 373, 587
Trammell, S., Hines, D., Wheeler, J. C. 1993, ApJ 414, 21CrossRef
Wang, L., Wheeler, J. C., Li, Z., Clocchiatti, A., 1996, ApJ 467, 435CrossRef
Wang, L., Howell, A., Höflich, P., Wheeler, C. 2001, ApJ 550, 1030CrossRef
Wang, L., Baade, D., Höflich, P., Wheeler, C., Fransson, C., Lundqvist, P. 2002, ApJ, submitted
Wang, L., et al. 2002b, ApJ Let., in press & astro-ph/0205337
Wang, L., Baade, D., Höflich, P., Khokhlov, A, Wheeler, J. C., Kasen, D., Nugent, P., Perlmutter, S., Fransson, C., Lundqvist, P. 2003, ApJ 591, 1110CrossRef
Wang, L., Baade, D., Höflich, P., Wheeler, J. C., Kawabata, K., Nomoto, K. 2003, ApJ, submitted

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