Overview of the Orion Complex

TL;DR

The paper reviews the structure, star formation history, and feedback effects within the Orion Complex, highlighting its role as a nearby, well-studied star-forming region influencing its surrounding interstellar environment.

Contribution

It provides a comprehensive overview of the Orion Complex's structure, star formation processes, and feedback mechanisms, integrating recent observational data and contextualizing it within the Solar vicinity.

Findings

Orion has formed over ten thousand stars in multiple sub-groups.

Supernovae in Orion created a large super-bubble affecting surrounding clouds.

Feedback from stars influences ongoing star formation in the region.

Abstract

The Orion star formation complex is the nearest region of on-going star formation that continues to produce both low and high mass stars. Orion is discussed in the larger context of star formation in the Solar vicinity over the last 100 Myr. The Orion complex is located on the far side of the Gould's Belt system of clouds and young stars throughwhich our Solar systemis drifting. A review is given of the overall structure and properties of the Orion star forming complex, the best studied OB association. Over the last 12 Myr, Orion has given birth to at least ten thousand stars contained in a half dozen sub-groups and short-lived clusters. The Orion OB association has been the source of several massive, high-velocity run-away stars, including mu-Columbae and AE Aurigae. Some of Orion's most massive members died in supernova explosions that created the 300 pc diameter Orion / Eridanus super-bubble whose near wall may be as close as 180 pc. The combined effects of UV radiation, stellar winds, and supernovae have impacted surviving molecular clouds in Orion. The large Orion A, IC 2118 molecular clouds and dozens of smaller clouds strewn throughout the interior of the superbubble have cometary shapes pointing back towards the center of the Orion OB association. Most are forming stars in the compressed layers facing the bubble interior.