Supernova Research

Research Initiative - CAPIBARA Project

Introduction

Supernova Remnants (SNRs) are the expanding materials left after a supernova explosion. Supernovae are classified as either Core Collapse (massive stars) or Thermonuclear (white dwarf explosions), each producing different types of stellar remnants. SNRs allow us to study chemical element formation and contribute heavy metals to new stars. Their X-ray emissions also reveal the possible presence of neutron stars.

Research Focus

We aim to identify particles in the core of SNRs by studying their influence on shock waves.

Methods

X-ray observations and analysis.

Authors

Hongda Zheng

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This project is part of the scientific program by the CAPIBARA Collaboration. However, we are open to any collaboration regarding the science outcomes of the missions (contact us!) and we will make all of our data public for the research community.