Year: 2016
Type: article
Abstract: Context. The structure of interstellar medium can be characterised at large scales in terms of its global statistics (e.g. power spectra) and at small scales by the properties of individual cores. Interest has been increasing in structures at intermediate scales, resulting in a number of methods being developed for the analysis of filamentary structures.
Source: Astronomy and Astrophysics
Author: M. Juvela
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Funder: Academy of Finland
Award: G2095330141
OpenAlex ID: W2463561754
