OGLE-2013-SN-079: a lonely supernova consistent with a helium shell detonation
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Authors
Inserra, C
Sim, S. A
Wyrzykowski, L
Smartt, S. J
Fraser, M
Nicholl, M
Shen, K. J.
Jerkstrand, A.
Gal-Yam, A.
Howell, D. A.
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American Astronomical Society
Abstract
We present observational data for a peculiar supernova discovered by the OGLE-IV survey and followed by the
Public ESO Spectroscopic Survey for Transient Objects. The inferred redshift of z = 0.07 implies an absolute
magnitude in the rest-frame I-band of MI ∼ −17.6 mag. This places it in the luminosity range between normal
Type Ia SNe and novae. Optical and near infrared spectroscopy reveal mostly Ti and Ca lines, and an unusually
red color arising from strong depression of flux at rest wavelengths <5000 Å. To date, this is the only reported
SN showing Ti-dominated spectra. The data are broadly consistent with existing models for the pure detonation
of a helium shell around a low-mass CO white dwarf and “double-detonation” models that include a secondary
detonation of a CO core following a primary detonation in an overlying helium shell.
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The Astrophysical Journal Letters
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