TL;DR
This review summarizes current knowledge about the Gould belt, a nearby stellar-gas complex, covering its stellar populations, gas components, kinematics, and theories on its origin and evolution.
Contribution
It provides a comprehensive synthesis of observational data and models regarding the structure, composition, and formation scenarios of the Gould belt.
Findings
Characterized stellar populations and gas components of the Gould belt.
Discussed kinematic features and origin scenarios.
Summarized recent observational and theoretical advances.
Abstract
This review is devoted to studies of the Gould belt and the Local system. Since the Gould belt is the giant stellar-gas complex closest to the sun, its stellar component is characterized, along with the stellar associations and diffuse clusters, cold atomic and molecular gas, high-temperature coronal gas, and dust contained in it. Questions relating to the kinematic features of the Gould belt are discussed and the most interesting scenarios for its origin and evolution are examined.
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