ASASSN-15pz: Revealing Significant Photometric Diversity among 2009dc-like, Peculiar SNe Ia

We report comprehensive multi-wavelength observations of a peculiar Type Ia-like supernova (“SN Ia-pec”) ASASSN-15pz. ASASSN-15pz is a spectroscopic “twin” of SN 2009dc, a so-called “Super-Chandrasekhar-mass” SN, throughout its evolution, but it has a peak luminosity that is dimmer and comparable to...

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Published in:The Astrophysical journal 2019-07, Vol.880 (1), p.35
Main Authors: Chen, Ping, Dong, Subo, Katz, Boaz, Kochanek, C. S., Kollmeier, Juna A., Maguire, K., Phillips, M. M., Prieto, J. L., Shappee, B. J., Stritzinger, M. D., Bose, Subhash, Brown, Peter J., Holoien, T. W.-S., Galbany, L., Milne, Peter A., Morrell, Nidia, Piro, Anthony L., Stanek, K. Z., Thompson, Todd A., Young, D. R.
Format: Article
Language:English
Subjects:
Astrophysics
Biological evolution
Extinction
Galaxies
Light curve
Luminosity
Phenomenology
Supernova
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Summary:We report comprehensive multi-wavelength observations of a peculiar Type Ia-like supernova (“SN Ia-pec”) ASASSN-15pz. ASASSN-15pz is a spectroscopic “twin” of SN 2009dc, a so-called “Super-Chandrasekhar-mass” SN, throughout its evolution, but it has a peak luminosity that is dimmer and comparable to the SN 1991T sub-class of SNe Ia at the luminous end of the normal width-luminosity relation. The synthesized 56 Ni mass of is also substantially less than that found for several 2009dc-like SNe. Previous well-studied 2009dc-like SNe have generally suffered from large and uncertain amounts of host-galaxy extinction, which is negligible for ASASSN-15pz. Based on the color of ASASSN-15pz, we estimate a host extinction for SN 2009dc of and confirm its high luminosity ( ). The 2009dc-like SN population, which represents ∼1% of SNe Ia, exhibits a range of peak luminosities, and do not fit onto the tight width-luminosity relation. Their optical light curves also show significant diversity of late-time (≳50 days) decline rates. The nebular-phase spectra provide powerful diagnostics to identify the 2009dc-like events as a distinct class of SNe Ia. We suggest referring to these sources using the phenomenology-based “2009dc-like SN Ia-pec” instead of “Super-Chandrasekhar SN Ia,” which is based on an uncertain theoretical interpretation.
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/ab2630