The Unification of Asymmetry Signatures of Type Ia Supernovae

We present a compilation of the geometry measures acquired using optical and IR spectroscopy and optical spectropolarimetry to probe the explosion geometry of Type Ia supernovae (SNe Ia). Polarization measurements are sensitive to asymmetries in the plane of the sky, whereas line profiles in nebular...

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Bibliographic Details
Published in:Astrophysical journal. Letters 2010-12, Vol.725 (2), p.L167-L171
Main Authors: Maund, Justyn R, Höflich, Peter, Patat, Ferdinando, Wheeler, J. Craig, Zelaya, Paula, Baade, Dietrich, Wang, Lifan, Clocchiatti, Alejandro, Quinn, Jason
Format: Article
Language:English
Subjects:
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
ASYMMETRY
BINARY STARS
ELEMENTS
EMISSION
ERUPTIVE VARIABLE STARS
EVOLUTION
EXPLOSIONS
INFRARED SPECTRA
MASS
NONMETALS
OXYGEN
POLARIZATION
SPECTRA
STAR EVOLUTION
STARS
SUPERNOVAE
VARIABLE STARS
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Summary:We present a compilation of the geometry measures acquired using optical and IR spectroscopy and optical spectropolarimetry to probe the explosion geometry of Type Ia supernovae (SNe Ia). Polarization measurements are sensitive to asymmetries in the plane of the sky, whereas line profiles in nebular phase spectra are expected to trace asymmetries perpendicular to the plane of the sky. The combination of these two measures can overcome their respective projection effects, completely probing the structures of these events. For nine normal SNe Ia, we find that the polarization of Si II Delta *l6355 at 5 days before maximum (p Si II ) is well correlated with its velocity evolution (), implying that is predominantly due to the asymmetry of the SNe. We find only a weak correlation between the polarization of Si II and the reported velocities (v neb) for peak emission of optical Fe II and Ni II lines in nebular spectra. Our sample is biased, with polarization measurements being only available for normal SNe that subsequently exhibited positive (i.e., redshifted) v neb. In unison these indicators are consistent with an explosion in which the outer layers are dominated by a spherical oxygen layer, mixed with an asymmetric distribution of intermediate-mass elements. The combination of spectroscopic and spectropolarimetric indicators suggests a single geometric configuration for normal SNe Ia, with some of the diversity of observed properties arising from orientation effects.
ISSN:2041-8205
2041-8213
DOI:10.1088/2041-8205/725/2/L167