iPTF14atg, a subluminous peculiar Type Ia supernova (SN Ia) similar to SN 2002es, is the first SN Ia for which a strong UV flash was observed in the early-time light curves. This has been interpreted as evidence for a single-degenerate (SD) progenitor system where such a signal is expected from interactions between the SN ejecta and the non-degenerate companion star. Here, we compare synthetic observables of multi-dimensional state-of-the-art explosion models for different progenitor scenarios to the light curves and spectra of iPTF14atg. From our models, we have difficulties explaining the spectral evolution of iPTF14atg within the SD progenitor channel. In contrast, we find that a violent merger of two carbon-oxygen white dwarfs with 0.9 and 0.76 solar masses, respectively, provides an excellent match to the spectral evolution of iPTF14atg from 10d before to several weeks after maximum light. Our merger model does not naturally explain the initial UV flash of iPTF14atg. We discuss several possibilities like interactions of the SN ejecta with the circum-stellar medium and surface radioactivity from a He ignited merger that may be able to account for the early UV emission in violent merger models.
@article{arxiv.1604.05730,
title = {The peculiar Type Ia supernova iPTF14atg: Chandrasekhar-mass explosion or violent merger?},
author = {M. Kromer and C. Fremling and R. Pakmor and S. Taubenberger and R. Amanullah and S. B. Cenko and C. Fransson and A. Goobar and G. Leloudas and F. Taddia and F. K. Roepke and I. R. Seitenzahl and S. A. Sim and J. Sollerman},
journal= {arXiv preprint arXiv:1604.05730},
year = {2016}
}
Comments
12 pages, 7 figures, accepted for publication in MNRAS