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6533b870fe1ef96bd12cf7a9

RESEARCH PRODUCT

Laboratory unraveling of matter accretion in young stars

Guilhem RevetSophia N. ChenRosaria BonitoBenjamin KhiarEvgeny FilippovCostanza ArgiroffiDrew P. HigginsonSalvatore OrlandoJérôme BéardMarius BlecherMarco BorghesiKonstantin BurdonovDimitri KhaghaniKealan NaughtonHenri PépinOliver PortugallRaphael RiquierRafael RodriguezSergei N. RyazantsevIgor Yu. SkobelevAlexander SolovievOswald WilliSergey PikuzAndrea CiardiJulien Fuchs

subject

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

description

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

yearjournalcountryeditionlanguage
2017-11-01
10.1126/sciadv.1700982https://hal-cea.archives-ouvertes.fr/cea-01887635
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