The role of cooling dust particles in gravitational turbulent protoplanetary disks
The static structure of a turbulent self-gravitational disk is investigated based on the effect of cooling due to the presence of dust particles. In agreement with the numerical simulations of self-gravitational disks that have been done so far, the cumulative parameter is assumed to be on the thres...
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| Format: | Article |
| Language: | English |
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Isfahan University of Technology
2019-03-01
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| Series: | Iranian Journal of Physics Research |
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| Online Access: | http://ijpr.iut.ac.ir/browse.php?a_code=A-10-3056-1&slc_lang=en&sid=1 |