Teşileanu, O. and Mignone, A. and Massaglia, S. (2009) YSO jets: MHD simulations with radiative cooling. Il nuovo cimento C, 32 (2). pp. 187-191. ISSN 1826-9885
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Abstract
The new High Power Computing facilities available for the scientific community allowed the use of increasingly complex codes for the numerical simulation of physical processes. Recent magnetohydrodynamic (MHD) simulations of astrophysical jets could finally include non-ideal effects, such as the radiative cooling we will discuss in this work in the context of protostellar jets. This makes the simulations more reliable and, with the recent improvements in available observational data, will provide a valuable tool for model discrimination. From 2D adaptivemesh refinement (AMR) simulations, synthetic surface brightness maps for the line emissions are computed, to be compared with observations.
| Item Type: | Article |
|---|---|
| Uncontrolled Keywords: | Jets, outflows, and bipolar flows ; Magnetohydrodynamic and fluid equation ; Atomic processes and interactions ; Numerical simulation; solution of equations |
| Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
| Depositing User: | Marina Spanti |
| Date Deposited: | 25 Mar 2020 15:28 |
| Last Modified: | 25 Mar 2020 15:28 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/16541 |
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