Modelling ripples in Orion with coupled dust dynamics and radiative transfer

T. Hendrix; R. Keppens; P. Camps

doi:10.1051/0004-6361/201425498

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Volume 575 (March 2015)

A&A, 575 (2015) A110

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Fig. 1

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Observation of the ripples in Orion at 8 μm, taken with the Spitzer Infrared Array Camera. The spatial wavelength λ, the orientation of the phase velocity V_φ, and the linear regime length L_lin are identified in the image. Credit: Fig. 1 from Berné & Matsumoto , reproduced by permission of the AAS.

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