Different dust and gas radial extents in protoplanetary disks: consistent 
models of grain growth and CO emission

Facchini, S.; Birnstiel, T.; Bruderer, S.; Van Dishoeck, E. F.

doi:10.1051/0004-6361/201630329

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Different dust and gas radial extents in protoplanetary disks: consistent models of grain growth and CO emission

MPS-Authors

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

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Bruderer, 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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Facchini, S., Birnstiel, T., Bruderer, S., & Van Dishoeck, E. F. (2017). Different dust and gas radial extents in protoplanetary disks: consistent models of grain growth and CO emission. Astronomy & Astrophysics, 605:. doi:10.1051/0004-6361/201630329.

引用: https://hdl.handle.net/11858/00-001M-0000-002E-51D5-D

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