Velocity structure of the 50 pc long NGC 6334 filamentary cloud: Hints of multiple compressions and their impact on the cloud properties

Velocity structure of the 50 pc long NGC 6334 filamentary cloud: Hints of multiple compressions and their impact on the cloud properties

Context. The interstellar medium is observed to be organized in filamentary structures, and in neutral (H I) and ionized (H II) bubbles. The expanding nature of these bubbles shapes the surrounding medium and possibly plays a role in the formation and evolution of the interstellar filaments. The imp...

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Bibliographic Details
Main Authors: André, P. (Author), Arzoumanian, D. (Author), Chun-Yuan Chen, M. (Author), Inutsuka, S.-I (Author), Kohno, M. (Author), Mena'shchikov, A. (Author), Misugi, Y. (Author), Russeil, D. (Author), Sánchez-Monge, Á (Author), Schilke, P. (Author), Zavagno, A. (Author)
Format: Article
Language:English
Published: EDP Sciences 2022
Subjects:
Clouds
Environmental impact
Interstellar medias
Ionization of gases
ISM : clouds
ISM: clouds
ISM: kinematics and dynamics
ISM: Kinematics and dynamics
ISM: structure
Kinematics
Molecular clouds
Power spectrum
Stars
Stars formation
Stars: formation
Structural properties
Submillimeter: ISM
Submillimetre
Velocity
Velocity gradients
Velocity structure
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