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High gas-to-dust size ratio indicating efficient radial drift in the mm-faint CX Tauri disk

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Facchini,  S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Van Dishoeck,  E. F.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Cazzoletti,  P.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Facchini, S., Van Dishoeck, E. F., Manara, C. F., Tazzari, M., Maud, L., Cazzoletti, P., et al. (2019). High gas-to-dust size ratio indicating efficient radial drift in the mm-faint CX Tauri disk. Astronomy and Astrophysics, 626: L2. doi:10.1051/0004-6361/201935496.


Cite as: https://hdl.handle.net/21.11116/0000-0004-8301-6
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