1991T-like Supernovae

TL;DR

This study analyzes the properties of 1991T-like supernovae, revealing their close relation to other luminous Type Ia supernovae and suggesting a continuum of characteristics influenced by nickel mixing and progenitor systems.

Contribution

It provides a detailed observational comparison of 1991T-like supernovae with related subclasses, proposing they form a continuum influenced by nickel mixing and progenitor origin.

Findings

1991T-like supernovae are closely related to slow-declining Type Ia supernovae.

Differences are mainly due to nickel mixing affecting spectra and luminosity.

1991T-like events may originate from single-degenerate progenitor systems.

Abstract

Understanding the nature of the luminous 1991T-like supernovae is of great importance to supernova cosmology as they are likely to have been more common in the early universe. In this paper we explore the observational properties of 1991T-like supernovae to study their relationship to other luminous, slow-declining Type~Ia supernovae (SNe Ia). From the spectroscopic and photometric criteria defined in Phillips et al. (1992), we identify 17 1991T-like supernovae from the literature. Combining these objects with ten 1991T-like supernovae from the Carnegie Supernova Project-II, the spectra, light curves, and colors of these events, along with their host galaxy properties, are examined in detail. We conclude that 1991T-like supernovae are closely related in essentially all of their UV, optical, and near-infrared properties -- as well as their host galaxy parameters -- to the slow-declining subset of Branch core-normal supernovae and to the intermediate 1999aa-like events, forming a continuum of luminous SNe Ia. The overriding difference between these three subgroups appears to be the extent to which $^{56}$Ni mixes into the ejecta, producing the pre-maximum spectra dominated by Fe III absorption, the broader UV light curves, and the higher luminosities that characterize the 1991T-like events. Nevertheless, the association of 1991T-like SNe with the rare Type Ia CSM supernovae would seem to run counter to this hypothesis, in which case 1991T-like events may form a separate subclass of SNe Ia, possibly arising from single-degenerate progenitor systems.