Issue |
EAS Publications Series
Volume 75-76, 2015
Conditions and Impact of Star Formation
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Page(s) | 177 - 180 | |
Section | Star Formation: Physical and Chemical Conditions, Feedback | |
DOI | https://doi.org/10.1051/eas/1575032 | |
Published online | 20 May 2016 |
Conditions and Impact of Star Formation
R. Simon, R. Schaaf and J. Stutzki (eds)
EAS Publications Series, 75–76 (2015) 177-180
R. Simon, R. Schaaf and J. Stutzki (eds)
EAS Publications Series, 75–76 (2015) 177-180
Filamentary Structure of the Orion A Molecular Cloud
I.Physikalisches Institut, Universität zu Köln, Cologne, Germany
Interstellar filaments pervade molecular clouds on all scales providing a bridge between the gas with relatively low densities and the dense clumps. In this work, we characterize various physical properties of filaments in the Orion A molecular cloud using preliminary datasets from the CARMA Orion project. We use an automated filament finding algorithm, DisPerSE, on 3D datacubes, and custom characterization algorithms.
© EAS, EDP Sciences, 2016