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Polytropic models of filamentary molecular clouds: structure, stability and magnetic fields

Journal
Date Issued
2017
Author(s)
•
Abstract
Recent observations made by the Herschel Space Observatory and the Planck Satellite have shown that molecular clouds are made by networks of filaments, shaped by interstellar turbulence and magnetic fields. We analyse the stability of filamentary molecular clouds with the help of cylindrical polytropic models with helical magnetic fields.
Volume
88
Start page
751
Uri
Url
Issn Identifier
0037-8720
Ads BibCode
2017MmSAI..88..751T
Rights
open.access
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