Laboratory unraveling of matter accretion in young stars

Accretion dynamics in the formation of young stars is still a matter of debate because of limitations in observations and modeling. Through scaled laboratory experiments of collimated plasma accretion onto a solid in the presence of a magnetic field, we open a first window on this phenomenon by trac...

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Detalhes bibliográficos
Publicado no:Sci Adv
Principais autores: Revet, Guilhem, Chen, Sophia N., Bonito, Rosaria, Khiar, Benjamin, Filippov, Evgeny, Argiroffi, Costanza, Higginson, Drew P., Orlando, Salvatore, Béard, Jérôme, Blecher, Marius, Borghesi, Marco, Burdonov, Konstantin, Khaghani, Dimitri, Naughton, Kealan, Pépin, Henri, Portugall, Oliver, Riquier, Raphael, Rodriguez, Rafael, Ryazantsev, Sergei N., Yu. Skobelev, Igor, Soloviev, Alexander, Willi, Oswald, Pikuz, Sergey, Ciardi, Andrea, Fuchs, Julien
Formato: Artigo
Idioma:Inglês
Publicado em: American Association for the Advancement of Science 2017
Assuntos:
Research Articles
Acesso em linha:https://ncbi.nlm.nih.gov/pmc/articles/PMC5665592/
https://ncbi.nlm.nih.gov/pubmed/29109974
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1126/sciadv.1700982
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