The Unprecedented 2012 Outburst of SN 2009ip: A Luminous Blue Variable Becomes a True Supernova

TL;DR

SN 2009ip, previously thought to be an LBV eruption, actually underwent a core-collapse supernova in 2012, showing typical SN II spectral features and brightness evolution, indicating a true supernova event during an LBV phase.

Contribution

This paper provides the first spectroscopic evidence that SN 2009ip was a genuine core-collapse supernova, not just an LBV eruption, with detailed velocity measurements and spectral evolution.

Findings

Spectra showed broad P-Cygni lines with velocities up to -13,000 km/s.

The supernova brightened rapidly after initial faintness, reaching M_R=-18 mag.

Spectral features transitioned from LBV-like to typical SN IIn signatures.

Abstract

Some reports of supernova (SN) discoveries turn out not to be true core-collapse explosions. One such case was SN 2009ip, which was recognized to be a luminous blue variable (LBV) eruption. This source had a massive hot progenitor star identified in pre-explosion data, it had documented evidence of pre-outburst variability, and it was subsequently discovered to have a 2nd outburst in 2010. This same source rebrightened again in 2012, and early spectra showed the same narrow-line profiles as before, suggesting another LBV-like eruption. We present new photometry and spectroscopy of SN 2009ip, indicating that it has transitioned into a true SN. The most striking discovery in these data is that unlike previous reports, the spectrum exhibited Balmer lines with very broad P-Cygni profiles characteristic of normal Type II supernovae (SNe II), in addition to narrow emission lines seen in SNe IIn and LBVs. Emission components have FWHM 8000 km/s, while the P-Cygni absorption component has blue wings extending to -13,000 km/s. These velocities are typical of SNe II, but have never been associated with emission lines from a nonterminal LBV-like eruption. Initially, the peak absolute magnitude seemed fainter than that of normal SNe. However, after a brief period of fading, the source quickly brightened again to M_R=-17.5 mag over a couple days. The broad lines mostly disappeared, and the spectrum began to resemble the early optically thick phases of SNe IIn. Two weeks later the source leveled off near -18 mag, after which broad emission lines again developed in the spectrum as the source faded. We conclude that the 2012 outburst of SN 2009ip was the result of a true core-collapse SN IIn that occured when the progenitor star was in an LBV-like outburst phase, and where the SN was initially faint and then rapidly brightened due to interaction with circumstellar material (abridged).