# Observational Properties of Thermonuclear Supernovae

## TL;DR

This review summarizes the observational properties of thermonuclear supernovae, especially type Ia, highlighting their significance in cosmology and chemical enrichment, while discussing current uncertainties in their progenitors and explosion mechanisms.

## Contribution

It provides a comprehensive overview of the observational characteristics and diversity of thermonuclear supernovae, emphasizing recent discoveries and ongoing challenges.

## Key findings

- Type Ia supernovae are key standard candles for cosmology.
- SN Ia progenitors and explosion mechanisms remain not fully understood.
- Recent observations reveal greater diversity in thermonuclear supernovae than previously recognized.

## Abstract

The explosive death of a star as a supernova is one of the most dramatic events in the Universe. Supernovae have an outsized impact on many areas of astrophysics: they are major contributors to the chemical enrichment of the cosmos and significantly influence the formation of subsequent generations of stars and the evolution of galaxies. Here we review the observational properties of thermonuclear supernovae, exploding white dwarf stars resulting from the stellar evolution of low-mass stars in close binary systems. The best known objects in this class are type Ia supernovae (SN Ia), astrophysically important in their application as standardisable candles to measure cosmological distances and the primary source of iron group elements in the Universe. Surprisingly, given their prominent role, SN Ia progenitor systems and explosion mechanisms are not fully understood; the observations we describe here provide constraints on models, not always in consistent ways. Recent advances in supernova discovery and follow-up have shown that the class of thermonuclear supernovae includes more than just SN Ia, and we characterise that diversity in this review.