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Laboratory modeling of jets from young stars using plasma focus facilities

†  a, b,  c,  d
a Lebedev Physical Institute, Russian Academy of Sciences, Leninsky prosp. 53, Moscow, 119991, Russian Federation
b Moscow Institute of Physics and Technology (National Research University), Institutskii per. 9, Dolgoprudny, Moscow Region, 141701, Russian Federation
c National Research Centre ‘Kurchatov Institute’, pl. akad. Kurchatova 1, Moscow, 123182, Russian Federation
d Lomonosov Moscow State University, Shternberg State Astronomical Institute, Universitetskii prosp. 13, Moscow, 119889, Russian Federation

Jets from young stars are used as an example to review how laboratory modeling enables advancement in understanding the main physical processes responsible for the formation and stability of these amazing objects. The discussion focuses on the options for modeling jet emissions in a laboratory experiment at the PF-3 facility at the National Research Center Kurchatov Institute. Many properties of the flows obtained using this experimental setup are consistent with the main features of jets from young stars.

Fulltext pdf (6 MB)
Fulltext is also available at DOI: 10.3367/UFNe.2021.12.039130
Keywords: jets from young stars, laboratory simulation, plasma focus
PACS: 52.58.Lq, 97.21.+a, 98.38.Fs (all)
DOI: 10.3367/UFNe.2021.12.039130
URL: https://ufn.ru/en/articles/2023/4/a/
001099929700001
2-s2.0-85175976900
2023PhyU...66..327B
Citation: Beskin V S, Krauz V I, Lamzin S A "Laboratory modeling of jets from young stars using plasma focus facilities" Phys. Usp. 66 327–359 (2023)
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Received: 16th, August 2021, revised: 14th, December 2021, 20th, December 2021

Îðèãèíàë: Áåñêèí Â Ñ, Êðàóç Â È, Ëàìçèí Ñ À «Ëàáîðàòîðíîå ìîäåëèðîâàíèå ñòðóéíûõ âûáðîñîâ èç ìîëîäûõ çâ¸çä íà óñòàíîâêàõ ñ ïëàçìåííûì ôîêóñîì» ÓÔÍ 193 345–381 (2023); DOI: 10.3367/UFNr.2021.12.039130

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