VLT Spectropolarimetry of the Type Ia SN2005ke - A step towards understanding subluminous events

TL;DR

This study presents spectropolarimetric observations of subluminous Type Ia SN2005ke, revealing significant asymmetry and polarization features that inform models of its explosion mechanism and progenitor system.

Contribution

It provides detailed spectropolarimetric data of a subluminous Type Ia supernova and interprets these findings within explosion and progenitor models, highlighting asymmetry and polarization characteristics.

Findings

SN2005ke shows high continuum polarization, peaking at ~0.7%.

The supernova exhibits a dominant axis in polarization, indicating global asymmetry.

Results suggest a possible origin from a rapidly rotating single-degenerate or double-degenerate system.

Abstract

We performed optical spectropolarimetric observations of the subluminous Type Ia SN2005ke at 3 epochs (days -8, -7, and +76). The explosion properties are derived by comparing the data to explosion and radiation transfer models. The SN shows polarimetric properties that are very similar to the only other subluminous event for which spectropolarimetry is available, i.e. SN1999by. The data present a very marked dominant axis, which is shared by both the continuum and lines such as SiII 6355, suggesting that the relatively large, global asymmetry is common to the photosphere and the line-forming region. The maximum polarization degree observed in the SiII 6355 absorption reaches 0.39+/-0.08%. At variance with what is seen in core-normal Type Ia, SN2005ke displays significant continuum polarization, which grows from the blue to the red and peaks at about 7000 A, reaching ~0.7%. The properties of the polarization and flux spectra can be understood within the framework of a subluminous delayed-detonation (DD), or pulsating DD scenario, or WD mergers. The difference in appearance with respect to core-normal SNe Ia is caused by low photospheric temperatures in combination with layers of unburned C, and more massive layers of the products of explosive C and O burning. The comparatively high level of continuum polarization is explained in terms of a significant global asymmetry (~15%), which is well reproduced by an oblate ellipsoidal geometry. Our results suggest that SN2005ke arose either from a single-degenerate system in which the WD is especially rapidly rotating, close to the break-up velocity, or from a double-degenerate merger. Based on the current polarization data, we cannot distinguish between these two possibilities.