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Development of 1D Non-ideal MHD Simulation Code Towards understanding Long-term Evolution of Protoplanetary Disk

We developed a one-dimensional magnetohydrodynamic (MHD) simulation code to investigate the long-term evolution of protoplanetary disks with low computational cost. In this simulation code, the physical processes necessary for protostellar formation and protoplanetary disk evolution, such as magneti...

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I tiakina i:
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Ngā kaituhi matua: Yudai Kobayashi, Daisuke Takaishi, Yusuke Tsukamoto, Shantanu Basu
Hōputu: Artigo
Reo:Inglês
I whakaputaina: IOP Publishing 2025-01-01
Rangatū:The Astrophysical Journal
Ngā marau:
Urunga tuihono:https://doi.org/10.3847/1538-4357/adf4ea
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