Measuring filament orientation: a new quantitative, local approach

C. E. Green, J. R. Dawson, M. R. Cunningham, P. A. Jones, G. Novak, L. M. Fissel

    Research output: Contribution to journalArticlepeer-review

    1 Citation (Scopus)

    Abstract

    The relative orientation between filamentary structures in molecular clouds and the ambient magnetic field provides insight into filament formation and stability. To calculate the relative orientation, a measurement of filament orientation is first required. We propose a new method to calculate the orientation of the one-pixel-wide filament skeleton that is output by filament identification algorithms such as filfinder. We derive the local filament orientation from the direction of the intensity gradient in the skeleton image using the Sobel filter and a few simple post-processing steps. We call this the "Sobel-gradient method." The resulting filament orientation map can be compared quantitatively on a local scale with the magnetic field orientation map to then find the relative orientation of the filament with respect to the magnetic field at each point along the filament. It can also be used for constructing radial profiles for filament width fitting. The proposed method facilitates automation in analyses of filament skeletons, which is imperative in this era of "big data."

    Original languageEnglish
    Article number6
    Pages (from-to)1-8
    Number of pages8
    JournalThe Astrophysical Journal. Supplement Series
    Volume232
    Issue number1
    DOIs
    Publication statusPublished - 1 Sept 2017

    Keywords

    • ISM: structure
    • methods: data analysis
    • methods: statistical
    • stars: formation
    • techniques: image processing

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