A 3D Map of the Local Bubble’s Magnetic Field

Author(s)

Theo O'Neill, Alyssa Goodman, Juan Soler, Jiwon Jesse Han, Joao Alves, Catherine Zucker

Abstract

We present a 3D map of magnetic field orientation on the surface of the Local Bubble, a low-density cavity in the nearby interstellar medium created by supernovae. This map is the first of its kind to fully chart magnetic fields over an observed superbubble. Recent work mapping the 3D shape and dynamics of the Local Bubble has revealed that the formation of all young stars within 200 pc of the Sun was triggered by the Bubble’s rapid expansion (Zucker et al. 2022). The exact mechanics of this expansion, and the role that magnetic fields in the surrounding interstellar medium have played in regulating its evolution, is not yet clear. By combining detailed models of the Bubble’s geometry (derived from 3D dust mapping, Pelgrims et al. 2020) with the assumption that magnetic field vectors are tangent to the Bubble’s surface, we are able to infer the 3D magnetic field orientation from Planck plane-of-the-sky dust polarization orientations. We analyze the relationship between the Bubble’s inferred magnetic field and background starlight polarimetry observations, and discuss how magnetic fields may have affected the dynamics of the Local Bubble and other nearby structures in the ISM.

Organisation(s)

Department of Astrophysics

External organisation(s)

University of Virginia, Max-Planck-Institut für Astronomie, Harvard-Smithsonian Center for Astrophysics, Space Telescope Science Institute

No. of pages

1

Publication date

01-2023

Austrian Fields of Science 2012

103003 Astronomy, 103004 Astrophysics

Portal url

https://ucris.univie.ac.at/portal/en/publications/a-3d-map-of-the-local-bubbles-magnetic-field(dda7540b-28aa-41f1-8895-6960b35abbea).html