Looking into the world of interacting supernovae
Anjasha Gangopadhyay

TL;DR
This paper reviews the diversity and complexities of interacting supernovae, emphasizing their importance in understanding massive star evolution, circumstellar environments, and the need for advanced observations and modeling.
Contribution
It provides a comprehensive overview of interacting supernovae types, their properties, and discusses recent observational and modeling challenges and advances.
Findings
Diverse types of interacting SNe include IIn, Ibn, and Icn.
High-cadence observations are vital for capturing early supernova interactions.
Modeling efforts are crucial for understanding progenitor systems and CSM structures.
Abstract
Interacting supernovae provide key insights into the mass-loss processes of massive stars and their circumstellar environments. By analyzing their photometric and spectroscopic properties, we can study the complex interactions between ejected material and circumstellar material (CSM). This paper highlights the diversity of interacting SNe, including Types IIn, Ibn, and Icn, and explores the challenges in understanding progenitor systems, CSM structures, and late-time evolution. Advances in high-cadence observations and modeling are crucial for improving our knowledge of these stellar explosions.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGamma-ray bursts and supernovae
