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Striations in the Taurus molecular cloud: Kelvin–Helmholtz instability or MHD waves?

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https://hal.archives-ouvertes.fr/hal-02317617
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Submitted on : Saturday, August 6, 2022 - 8:08:46 AM
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M. Heyer, P. Goldsmith, U. Yildiz, R. Snell, E. Falgarone, et al.. Striations in the Taurus molecular cloud: Kelvin–Helmholtz instability or MHD waves?. Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P - Oxford Open Option A, 2016, 461 (4), pp.3918-3926. ⟨10.1093/mnras/stw1567⟩. ⟨hal-02317617⟩

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