# The evolution of red supergiants to supernovae

## TL;DR

This study investigates how mass loss rates in red supergiants increase with stellar evolution, affecting supernova progenitor observations and potentially leading to underestimations of initial stellar mass.

## Contribution

It provides the first direct measurements showing mass loss rates ramp up significantly as RSGs evolve, impacting supernova progenitor analysis.

## Key findings

- Mass loss rates increase by a factor of 40 in evolved RSGs.
- Circumstellar extinction also increases with stellar evolution.
- Potential underestimation of progenitor mass by up to 9 solar masses.

## Abstract

With red supergiants (RSGs) predicted to end their lives as Type IIP core collapse supernova (CCSN), their behaviour before explosion needs to be fully understood. Mass loss rates govern RSG evolution towards SN and have strong implications on the appearance of the resulting explosion. To study how the mass-loss rates change with the evolution of the star, we have measured the amount of circumstellar material around 19 RSGs in a coeval cluster. Our study has shown that mass loss rates ramp up throughout the lifetime of an RSG, with more evolved stars having mass loss rates a factor of 40 higher than early stage RSGs. Interestingly, we have also found evidence for an increase in circumstellar extinction throughout the RSG lifetime, meaning the most evolved stars are most severely affected. We find that, were the most evolved RSGs in NGC2100 to go SN, this extra extinction would cause the progenitor's initial mass to be underestimated by up to 9M$_\odot$.