Massive star evolution: Luminous Blue Variables as unexpected Supernova progenitors

TL;DR

This study uses stellar evolution and atmospheric modeling to reveal that some massive stars, specifically LBVs, can directly explode as supernovae, challenging previous assumptions about their evolutionary stages.

Contribution

It demonstrates through models that LBVs can be direct supernova progenitors, a novel insight altering the understanding of massive star evolution.

Findings

Models show 20-25 Msun stars resemble LBVs before explosion

LBVs can be the end stage of massive star evolution

Type IIb supernovae may originate from LBV progenitors

Abstract

Stars more massive than about 8 Msun end their lives as a Supernova (SN), an event of fundamental importance Universe-wide. Theoretically, these stars have been expected to be either at the red supergiant, blue supergiant, or Wolf-Rayet stage before the explosion. We performed coupled stellar evolution and atmospheric modeling of stars with initial masses between 20 Msun and 120 Msun. We found that the 20 Msun and 25 Msun rotating models, before exploding as SN, have spectra that do not resemble any of the aforementioned classes of massive stars. Rather, they have remarkable similarities with rare, unstable massive stars known as Luminous Blue Variables (LBV). While observations show that some SNe seem to have had LBVs as progenitors, no theoretical model had yet predicted that a star could explode at this stage. Our models provide theoretical support for relatively low-luminosity LBVs exploding as SN in the framework of single stellar evolution. This is a significant shift in paradigm, meaning that a fraction of LBVs could be the end stage of massive star evolution, rather than a transitory evolutionary phase. We suggest that type IIb SN could have LBV as progenitors, and a prime example could be SN 2008ax.