Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Blecher, marius"'
Autor:
Revet, G., Chen, S. N., Bonito, Rosaria, Khiar, Benjamin, Filippov, E., argiroffi, costanza, Higginson, D.P., orlando, salvatore, Beard, J., Blecher, marius, Borghesi, Marco, Naughton, Kealan, Chen, Shenchang, Burdonov, Konstantin, Khaghani, D., Pépin, H., Portugall, O., Riquier, R., Rodriguez, Rafael, Ryazantsev, Sergey, Skobelev, I. Yu., Soloviev, A., Willi, Oswald, Pikuz, S. A., Ciardi, A., Fuchs, J.
Publikováno v:
Revet, G, Chen, S N, Bonito, R, Khiar, B, Filippov, E, argiroffi, C, Higginson, D P, orlando, S, Beard, J, Blecher, M, Borghesi, M, Naughton, K, Chen, S, Burdonov, K, Khaghani, D, Pépin, H, Portugall, O, Riquier, R, Rodriguez, R, Ryazantsev, S, Skobelev, I Y, Soloviev, A, Willi, O, Pikuz, S A, Ciardi, A & Fuchs, J 2017, ' Laboratory unraveling of matter accretion in young stars ', Science Advances, vol. 3, no. 11, e1700982, pp. 1-10 . https://doi.org/10.1126/sciadv.1700982
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,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2607::c33941ee0617a4c6cb7f903dec4a88ba
https://pure.qub.ac.uk/en/publications/d6ce0514-bd51-44f9-aefa-c85aa403eed5
https://pure.qub.ac.uk/en/publications/d6ce0514-bd51-44f9-aefa-c85aa403eed5
Autor:
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
Publikováno v:
Science Advances
Science Advances, American Association for the Advancement of Science (AAAS), 2017, 3 (11), pp.e1700982. ⟨10.1126/sciadv.1700982⟩
Science Advances, 2017, 3 (11), pp.e1700982. ⟨10.1126/sciadv.1700982⟩
Science Advances, American Association for the Advancement of Science (AAAS), 2017, 3 (11), pp.e1700982. ⟨10.1126/sciadv.1700982⟩
Science Advances, 2017, 3 (11), pp.e1700982. ⟨10.1126/sciadv.1700982⟩
When matter accretes onto a young star, a shell of dense material can form around the impact, reducing its x-ray emission.
Accretion dynamics in the formation of young stars is still a matter of debate because of limitations in observations and
Accretion dynamics in the formation of young stars is still a matter of debate because of limitations in observations and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid_dedup__::5624936ad8109f593f8558956e6b5589
https://hal-cea.archives-ouvertes.fr/cea-01887635
https://hal-cea.archives-ouvertes.fr/cea-01887635
Autor:
Revet G; Institute of Applied Physics, 46 Ulyanov Street, 603950 Nizhny Novgorod, Russia.; LULI (Laboratoire pour l'Utilisation des Lasers Intenses)-CNRS, École Polytechnique; Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris-Saclay; Sorbonne Universités, Universite Pierre et Marie Curie (UPMC) Paris 06, F-91128 Palaiseau cedex, France., Chen SN; Institute of Applied Physics, 46 Ulyanov Street, 603950 Nizhny Novgorod, Russia.; LULI (Laboratoire pour l'Utilisation des Lasers Intenses)-CNRS, École Polytechnique; Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris-Saclay; Sorbonne Universités, Universite Pierre et Marie Curie (UPMC) Paris 06, F-91128 Palaiseau cedex, France., Bonito R; INAF (Istituto Nazionale di Astrofisica)-Osservatorio Astronomico di Palermo, Palermo, Italy.; Dipartimento di Fisica e Chimica, Università di Palermo, Palermo, Italy., Khiar B; Sorbonne Universités, UPMC Paris 06, Observatoire de Paris, PSL (Paris Sciences et Lettre) Research University, CNRS, UMR 8112, LERMA (Laboratoire d'Etudes du Rayonnement et de la Matière en Astrophysique), F-75005 Paris, France., Filippov E; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow 115409, Russia.; Joint Institute for High Temperatures, RAS (Russian Academy of Sciences), Moscow 125412, Russia., Argiroffi C; Dipartimento di Fisica e Chimica, Università di Palermo, Palermo, Italy., Higginson DP; LULI (Laboratoire pour l'Utilisation des Lasers Intenses)-CNRS, École Polytechnique; Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris-Saclay; Sorbonne Universités, Universite Pierre et Marie Curie (UPMC) Paris 06, F-91128 Palaiseau cedex, France.; Lawrence Livermore National Laboratory, Livermore, CA 94551, USA., Orlando S; INAF (Istituto Nazionale di Astrofisica)-Osservatorio Astronomico di Palermo, Palermo, Italy., Béard J; LNCMI (Laboratoire National des Champs Magnétiques Intenses), UPR 3228, CNRS-UGA-UPS-INSA, Toulouse 31400, France., Blecher M; Institut für Laser- und Plasmaphysik, Heinrich-Heine-Universität Düsseldorf, D-40225 Düsseldorf, Germany., Borghesi M; Centre for Plasma Physics, Queen's University of Belfast, Belfast BT7 1NN, UK., Burdonov K; Institute of Applied Physics, 46 Ulyanov Street, 603950 Nizhny Novgorod, Russia., Khaghani D; GSI (Gesellschaft für Schwerionenforschung) Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany., Naughton K; Centre for Plasma Physics, Queen's University of Belfast, Belfast BT7 1NN, UK., Pépin H; INRS-EMT (Institut National de la Recherche Scientifique, Énergie, Matériaux et Télécommunication), Varennes, Québec, Canada., Portugall O; LNCMI (Laboratoire National des Champs Magnétiques Intenses), UPR 3228, CNRS-UGA-UPS-INSA, Toulouse 31400, France., Riquier R; LULI (Laboratoire pour l'Utilisation des Lasers Intenses)-CNRS, École Polytechnique; Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris-Saclay; Sorbonne Universités, Universite Pierre et Marie Curie (UPMC) Paris 06, F-91128 Palaiseau cedex, France.; CEA, DAM, DIF (Commissariat à l'Energie Atomique Energie Atomique, Direction des Applications Militaires Île de France), 91297 Arpajon, France., Rodriguez R; Departamento de Fisica de la Universidad de Las Palmas de Gran Canaria, E-35017 Las Palmas de Gran Canaria, Spain., Ryazantsev SN; Joint Institute for High Temperatures, RAS (Russian Academy of Sciences), Moscow 125412, Russia., Yu Skobelev I; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow 115409, Russia.; Joint Institute for High Temperatures, RAS (Russian Academy of Sciences), Moscow 125412, Russia., Soloviev A; Institute of Applied Physics, 46 Ulyanov Street, 603950 Nizhny Novgorod, Russia., Willi O; Institut für Laser- und Plasmaphysik, Heinrich-Heine-Universität Düsseldorf, D-40225 Düsseldorf, Germany., Pikuz S; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow 115409, Russia.; Joint Institute for High Temperatures, RAS (Russian Academy of Sciences), Moscow 125412, Russia., Ciardi A; Sorbonne Universités, UPMC Paris 06, Observatoire de Paris, PSL (Paris Sciences et Lettre) Research University, CNRS, UMR 8112, LERMA (Laboratoire d'Etudes du Rayonnement et de la Matière en Astrophysique), F-75005 Paris, France., Fuchs J; Institute of Applied Physics, 46 Ulyanov Street, 603950 Nizhny Novgorod, Russia.; LULI (Laboratoire pour l'Utilisation des Lasers Intenses)-CNRS, École Polytechnique; Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris-Saclay; Sorbonne Universités, Universite Pierre et Marie Curie (UPMC) Paris 06, F-91128 Palaiseau cedex, France.
Publikováno v:
Science advances [Sci Adv] 2017 Nov 01; Vol. 3 (11), pp. e1700982. Date of Electronic Publication: 2017 Nov 01 (Print Publication: 2017).