Abstract
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 λ6355 at 5 days before maximum (pSiII) is well correlated with its velocity evolution (ν̇ SiII), implying that ν̇ SiII is predominantly due to the asymmetry of the SNe. We find only a weak correlation between the polarization of SiII and the reported velocities (νneb) for peak emission of optical FeII and NiII lines in nebular spectra. Our sample is biased, with polarization measurements being only available for normal SNe that subsequently exhibited positive (i.e., redshifted) νneb. 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.
| Original language | English |
|---|---|
| Journal | Astrophysical Journal Letters |
| Volume | 725 |
| Issue number | 2 |
| Pages (from-to) | L167-L171 |
| Number of pages | 4 |
| DOIs | |
| Publication status | Published - 20 Dec 2010 |