Possible link between the power spectrum of interstellar filaments and the origin of the prestellar core mass function

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DOIResolve DOI: http://doi.org/10.1051/0004-6361/201526431
AuthorSearch for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for: ; Search for:
TypeArticle
Journal titleAstronomy and Astrophysics
ISSN0004-6361
Volume584
Article numberA111
SubjectFunctions; Power spectrum; Spectrum analysis; Stars; Turbulence; Characteristic indices; Compressible turbulence; Empirical correlations; Evolution; Gaussian-like distributions; ISM: structure; Mass functions; Stars: formation; Gravitation
Abstract
Publication date
PublisherEDP Sciences
LanguageEnglish
AffiliationNational Research Council Canada; National Science Infrastructure
Peer reviewedYes
NPARC number21277365
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Record identifier9a14f0b4-e13f-47ab-9f36-8db7d700eed9
Record created2016-03-09
Record modified2016-05-09
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