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Showing 1–4 of 4 results
Advanced filters: Author: Ralf S. Klessen Clear advanced filters

  • Extremely high-resolution simulations reveal that interstellar medium-type turbulence significantly deviates from classical magnetized turbulence models.

    • James R. Beattie
    • Christoph Federrath
    • Amitava Bhattacharjee
    Research
    Nature Astronomy
    Volume: 9, P: 1195-1205

  • A high-resolution simulation of interstellar turbulence determines the position and width of the transition from supersonic to subsonic turbulence, providing quantitative input for models of filament structure and star formation in molecular clouds.

    • Christoph Federrath
    • Ralf S. Klessen
    • James R. Beattie
    Research
    Nature Astronomy
    Volume: 5, P: 365-371

  • Statistical analysis of velocity fluctuations in the interstellar medium (ISM) of the Milky Way and NGC 4321 show that the motion of molecular gas over scales ranging from 0.1 to 1,000 pc is similar, and consistent with that generated by a combination of gravity and turbulence. ISM structure at one scale is therefore linked to structure at other scales.

    • Jonathan D. Henshaw
    • J. M. Diederik Kruijssen
    • Jiayi Sun
    Research
    Nature Astronomy
    Volume: 4, P: 1064-1071