On Identifying the Progenitors of Type Ia Supernovae
arXiv:1107.5729 · doi:10.1088/2041-8205/740/1/L18
Abstract
We propose two new means of identifying the main class of progenitors of Type Ia supernovae--single or double degenerate: (i) If the range of supernova properties is significantly determined by the range of viewing angles of non-spherically symmetric explosions, then the nature of the correlation between polarization and another property (for example, the velocity gradient) can be used to determine the geometry of the asymmetry and hence the nature of the progenitor, and (ii) in the double- but not in the single-degenerate case, the range in the observed properties (e.g., velocity gradients) is likely to increase with the amount of carbon seen in the ejecta.
10 pages, 2 figures; ApJL in press
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- Circumstellar Shell Formation in Symbiotic Recurrent Novae
- Asymmetries in SN 2014J Near Maximum Light Revealed Through Spectropolarimetry
- The Long-Term Secular Mass Accretion Rate of the Recurrent Nova T Pyxidis
- Evidence for Rapid Variability in the Optical Light Curve of the Type Ia SN 2014J
- Multi-epoch Spectropolarimetry of SN 2011fe