0000000001239118

AUTHOR

Henri Pépin

showing 2 related works from this author

Laboratory formation of a scaled protostellar jet by coaligned poloidal magnetic field

2014

International audience; Although bipolar jets are seen emerging from a wide variety of astrophysical systems, the issue of their formation and morphology beyond their launching is still under study. Our scaled laboratory experiments, representative of young stellar object outflows, reveal that stable and narrow collimation of the entire flow can result from the presence of a poloidal magnetic field whose strength is consistent with observations. The laboratory plasma becomes focused with an interior cavity. This gives rise to a standing conical shock from which the jet emerges. Following simulations of the process at the full astrophysical scale, we conclude that it can also explain recentl…

jetsPhysicsJet (fluid)MultidisciplinaryShock (fluid dynamics)Young stellar objectAstrophysics::High Energy Astrophysical PhenomenaFlow (psychology)PlasmaConical surfaceAstrophysics01 natural sciencesSIMULATIONS010305 fluids & plasmasMagnetic fieldCOLLIMATION[PHYS.COND.CM-S]Physics [physics]/Condensed Matter [cond-mat]/Superconductivity [cond-mat.supr-con]DISCOVERY0103 physical sciencesDG-TAURI010303 astronomy & astrophysicsACCRETION DISCSAstrophysics::Galaxy AstrophysicsDRIVEN JETS
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Laboratory unraveling of matter accretion in young stars

2017

When matter accretes onto a young star, a shell of dense material can form around the impact, reducing its x-ray emission.

HOTELECTRON THERMAL CONDUCTIONPLASMAT-TAURI STARSAstrophysics::High Energy Astrophysical PhenomenaMAGNETIC-FIELDCLOUDSSciAdv r-articlesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSIMULATIONSX-RAY-EMISSIONSettore FIS/05 - Astronomia E AstrofisicaGASPhysical SciencesAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Research ArticlesAstrophysics::Galaxy AstrophysicsResearch ArticleRADIATIVE SHOCKS
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