Nested shells reveal the rejuvenation of the Orion-Eridanus superbubble
B. B. Ochsendorf, A. G. A. Brown, J. Bally, and A. G. G. M. Tielens

TL;DR
This paper presents a comprehensive analysis of the Orion-Eridanus superbubble, revealing its complex nested shell structure, ongoing mass-loading processes, and implications for star formation and dust processing over tens of millions of years.
Contribution
It introduces a new, detailed model of the superbubble as a series of nested shells, based on combined observational data, highlighting ongoing rejuvenation and star formation processes.
Findings
Barnard's Loop is a complete bubble structure.
The superbubble contains nested shells expanding within each other.
Mass-loading and star formation are episodic, rejuvenating the superbubble.
Abstract
The Orion-Eridanus superbubble is the prototypical superbubble due to its proximity and evolutionary state. Here, we provide a synthesis of recent observational data from WISE and Planck with archival data, allowing to draw a new and more complete picture on the history and evolution of the Orion-Eridanus region. We discuss the general morphological structures and observational characteristics of the superbubble, and derive quantitative properties of the gas- and dust inside Barnard's Loop. We reveal that Barnard's Loop is a complete bubble structure which, together with the lambda Ori region and other smaller-scale bubbles, expands within the Orion-Eridanus superbubble. We argue that the Orion-Eridanus superbubble is larger and more complex than previously thought, and that it can be viewed as a series of nested shells, superimposed along the line of sight. During the lifetime of the…
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