work in progress

Necessary Conditions for the formation of filaments and star clusters in the cold neutral medium

Rachel Pillsworth, Ralph E. Pudritz

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  • arXiv link

    • Centered column density map of our Milky Way-like galaxy, with four kiloparsec length filaments highlighted, one in each quadrant. There are zooms in on each of these filaments to the sides.

    Filamentary Hierarchies and Superbubbles I: Characterizing filament properties across a simulated spiral galaxy

    Rachel Pillsworth, Erica Roscoe, Ralph E. Pudrits & Eric W. Koch

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  • arXiv link
    • Edge-on and face-on density projections (i.e. column density maps) of the Milky Way-like galaxy of Zhao et al. 2024.

    Filamentary Hierarchies and Superbubbles: Galactic Multiscale MHD Simulations of GMC to Star Cluster Formation

    Bo Zhao, Ralph E. Pudritz, Rachel Pillsworth, Hector Robinson, James Wadsley

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  • arXiv link

    • B-density scaling relation for the zoom-in simulations of Zhao et al. 2024.

    On the relation between magnetic field strength and gas density in the interstellar medium: A multiscale analysis

    Whitworth, D. J.; Srinivasan, S.; Pudritz, R. E.; Mac Low, M. -M.; Eadie, G.; Palau, A.; Soler, J. D.; Smith, R. J.; Pattle, K.; Robinson, H.; Pillsworth, R. et al.

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  • arXiv link