The Local Bubble is a Local Chimney: A New Model from 3D Dust Mapping
Theo J. O'Neill, Catherine Zucker, Alyssa A. Goodman, Gordian, Edenhofer

TL;DR
This paper presents a high-resolution 3D dust map revealing the irregular shape of the Local Bubble, including a chimney structure likely formed by supernova activity, with implications for understanding local interstellar medium dynamics.
Contribution
The study introduces a detailed 3D model of the Local Bubble's surface, highlighting its irregular shape and the presence of a chimney structure, based on new high-resolution dust mapping data.
Findings
The Local Bubble's surface peaks at 170 pc from the Sun.
The bubble has a typical thickness of 35 pc.
A chimney structure extends in the Galactic North, likely formed by supernova activity.
Abstract
Leveraging a high-resolution 3D dust map of the solar neighborhood from Edenhofer et al. (2024), we derive a new 3D model for the dust-traced surface of the Local Bubble, the supernova-driven cavity surrounding the Sun. We find that the surface of the Local Bubble is highly irregular in shape, with its peak extinction surface falling at an average distance of 170 pc from the Sun (spanning 70-600+ pc) with a typical thickness of 35 pc and a total dust-traced mass of . The Local Bubble displays an extension in the Galactic Northern hemisphere that is morphologically consistent with representing a "Local Chimney." We argue this chimney was likely created by the "bursting" of this supernova-driven superbubble, leading to the funneling of interstellar medium ejecta into the lower Galactic halo. We find that many well-known dust features and…
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Taxonomy
TopicsHistorical and Architectural Studies · Building materials and conservation · Planetary Science and Exploration
