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Filamentary structure formation in the Interstellar Radiation Field (ISRF)

Miao, Jingqi, Lieu, M., Cox, P., Kinnear, T.M., Cornwall, P. (2012) Filamentary structure formation in the Interstellar Radiation Field (ISRF). Proceedings of the International Astronomical Union, 8 (S292). p. 52. ISSN 1743-9213. (doi:10.1017/S1743921313000331) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:50016)

The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided.
Official URL:
http://dx.doi.org/10.1017/S1743921313000331

Abstract

A new mechanism is proposed for the formation of filament/core structure by ISRF and clumpy molecular cloud interaction. The derived characterizes of the filament/core network is consistent with that produced by the compressive forcing turbulence model.

Item Type: Article
DOI/Identification number: 10.1017/S1743921313000331
Uncontrolled keywords: ISM: clouds, ISM: evolution, ISM: structure
Subjects: Q Science > QB Astronomy > QB460 Astrophysics
Divisions: Divisions > Division of Natural Sciences > Physics and Astronomy
Depositing User: Giles Tarver
Date Deposited: 04 Aug 2015 14:52 UTC
Last Modified: 05 Nov 2024 10:35 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/50016 (The current URI for this page, for reference purposes)

University of Kent Author Information

Miao, Jingqi.

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Kinnear, T.M..

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