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dc.contributor.authorGogus, Ersin
dc.contributor.authorLU, FangJun
dc.contributor.authorBERNARDINI, Federico
dc.contributor.authorBUCCIANTINI, Niccolo'
dc.contributor.authorFEROCI, Marco
dc.contributor.authorFURST, Felix
dc.contributor.authorJI, Long
dc.contributor.authorPrescod-Weinstein, Chanda
dc.contributor.authorSANTANGELO, Andrea
dc.contributor.authorZane, Silvia
dc.contributor.authorFENG, Hua
dc.contributor.authorXU, RenXin
dc.contributor.authorDOROSHENKO, Victor
dc.contributor.authorBOZZO, Enrico
dc.contributor.authorPAUL, Biswajit
dc.contributor.authorMIKUSINCOVA, Romana
dc.contributor.authorMEREGHETTI, Sandro
dc.contributor.authorGungor, Can
dc.contributor.authorMANOUSAKIS, Antonios
dc.contributor.authorCaiazzo, Ilaria
dc.contributor.authorZELATI, Francesco Coti
dc.contributor.authorESPOSITO, Paolo
dc.contributor.authorGonzalez-Caniulef, Denis
dc.contributor.authorHeyl, Jeremy
dc.contributor.authorHuppenkothen, Daniela
dc.contributor.authorISRAEL, Gianluca
dc.contributor.authorLI, ZhaoSheng
dc.contributor.authorLIN, Lin
dc.contributor.authorMIGNANI, Roberto
dc.contributor.authorYounes, George
dc.contributor.authorTIENGO, Andrea
dc.contributor.authorXU, YuPeng
dc.contributor.authorWATTS, Anna
dc.contributor.authorZHANG, Shu
dc.contributor.authorZHAN, Shuang-Nan
dc.contributor.authorREA, Nanda
dc.contributor.authorORLANDINI, Mauro
dc.contributor.authorTAVERNA, Roberto
dc.contributor.authorTONG, Hao
dc.contributor.authorTurolla, Roberto
dc.contributor.authorBAGLIO, Cristina
dc.date.accessioned2021-03-04T13:34:16Z
dc.date.available2021-03-04T13:34:16Z
dc.date.issued2019
dc.identifier.citationSANTANGELO A., Zane S., FENG H., XU R., DOROSHENKO V., BOZZO E., Caiazzo I., ZELATI F. C. , ESPOSITO P., Gonzalez-Caniulef D., et al., "Physics and astrophysics of strong magnetic field systems with eXTP", SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, cilt.62, sa.2, 2019
dc.identifier.issn1674-7348
dc.identifier.otherav_7d121bce-6f26-40f3-8bcf-2ef095f51734
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/85496
dc.identifier.urihttps://doi.org/10.1007/s11433-018-9234-3
dc.description.abstractIn this paper we present the science potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies of strongly magnetized objects. We will focus on the physics and astrophysics of strongly magnetized objects, namely magnetars, accreting X-ray pulsars, and rotation powered pulsars. We also discuss the science potential of eXTP for QED studies. Developed by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Sciences, the eXTP mission is expected to be launched in the mid 2020s.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.subjectTemel Bilimler
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.subjectFizik
dc.titlePhysics and astrophysics of strong magnetic field systems with eXTP
dc.typeMakale
dc.relation.journalSCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
dc.contributor.departmentEberhard Karls University of Tubingen , ,
dc.identifier.volume62
dc.identifier.issue2
dc.contributor.firstauthorID106271


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