# Magnetism in the Brown Dwarf Regime

**Authors:** Melodie M. Kao, J. Sebastian Pineda, Peter Williams, Rakesh Yadav,, Denis Shulyak, Joachim Saur, David J. Stevenson, Sarah Schmidt, Adam, Burgasser, Gregg Hallinan, Kelle Cruz

arXiv: 1903.11586 · 2019-03-28

## TL;DR

This paper discusses the emerging field of brown dwarf magnetism, emphasizing its importance for understanding substellar magnetic phenomena and its potential to inform exoplanetary studies, with a focus on future observational and theoretical advancements.

## Contribution

It highlights the significance of brown dwarf magnetism research for broader astrophysical applications and outlines key scientific questions and necessary observational and modeling efforts.

## Key findings

- Magnetic dynamos in substellar objects are a key research area.
- Characterization of exo-aurora physics will advance understanding of planetary environments.
- Long-term monitoring and new observational capabilities are essential for progress.

## Abstract

A suite of discoveries in the last two decades demonstrate that we are now at a point where incorporating magnetic behavior is key for advancing our ability to characterize substellar and planetary systems. The next decade heralds the exciting maturation of the now-burgeoning field of brown dwarf magnetism, and investing now in brown dwarf magnetism will provide a key platform for exploring exoplanetary magnetism and habitability beyond the solar system. We anticipate significant discoveries including: the nature of substellar and planetary magnetic dynamos, the characterization of exo-aurora physics and brown dwarf magnetospheric environments, and the role of satellites in manifestations of substellar magnetic activity. These efforts will require significant new observational capabilities at radio and near infrared wavelengths, dedicated long-term monitoring programs, and committed support for the theoretical modeling efforts underpinning the physical processes of the magnetic phenomena

## Full text

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## Figures

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## References

63 references — full list in the complete paper: https://tomesphere.com/paper/1903.11586/full.md

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Source: https://tomesphere.com/paper/1903.11586