Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7156
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dc.contributor.authorEnrico, Bozzo-
dc.contributor.authorJinLu, Qu-
dc.contributor.authorPaul, Biswajit-
dc.contributor.author+ 152 Co-Authors-
dc.date.accessioned2019-02-12T18:17:26Z-
dc.date.available2019-02-12T18:17:26Z-
dc.date.issued2019-02-
dc.identifier.citationScience China Physics, Mechanics & Astronomy, Volume 62, AR 29506, 42 pp.en_US
dc.identifier.issn1674-7348-
dc.identifier.issn1869-1927(Online)-
dc.identifier.urihttp://hdl.handle.net/2289/7156-
dc.descriptionRestricted Access.en_US
dc.description.abstractIn this White Paper, we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring stars, supernova remnants, accreting white dwarfs, low and high mass X-ray binaries, radio quiet and radio-loud active galactic nuclei, tidal disruption events, and gamma-ray bursts. EXP will be excellently suited to study one common aspect of these objects: their often transient nature. Developed by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Science, the eXTP mission is expected to be launched in the mid-2020s.en_US
dc.language.isoenen_US
dc.publisherScience China Pressen_US
dc.relation.urihttps://ui.adsabs.harvard.edu//#abs/2019SCPMA..6229506I/abstracten_US
dc.relation.urihttps://arxiv.org/abs/1812.04023en_US
dc.relation.urihttps://doi.org/10.1007/s11433-017-9186-1en_US
dc.rights© Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2019en_US
dc.subjectspace research instrumentsen_US
dc.subjectnuclear astrophysicsen_US
dc.subjectflare starsen_US
dc.subjectaccretion and accretion disksen_US
dc.subjectmass loss and stellar windsen_US
dc.subjectX-ray binariesen_US
dc.titleObservatory science with eXTPen_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

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